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Journal articles on the topic 'Hot objects'

Author: Grafiati

Published: 3 June 2025

Last updated: 31 July 2025

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1

Wang, Yuxiao, Wenpeng Neng, Zhenao Wei, et al. "Precision-Enhanced Human-Object Contact Detection via Depth-Aware Perspective Interaction and Object Texture Restoration." Proceedings of the AAAI Conference on Artificial Intelligence 39, no. 8 (2025): 8187–95. https://doi.org/10.1609/aaai.v39i8.32883.

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Human-object contact (HOT) is designed to accurately identify the areas where humans and objects come into contact. Current methods frequently fail to account for scenarios where objects are frequently blocking the view, resulting in inaccurate identification of contact areas. To tackle this problem, we suggest using a perspective interaction HOT detector called PIHOT, which utilizes a depth map generation model to offer depth information of humans and objects related to the camera, thereby preventing false interaction detection. Furthermore, we use mask dilatation and object restoration techn

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Koen, C., D. O'Donoghue, D. Kilkenny, and R. S. Stobie. "The EC14026 Stars - Pulsating Hot Subdwarfs." Symposium - International Astronomical Union 185 (1998): 361–66. http://dx.doi.org/10.1017/s0074180900238941.

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The Edinburgh-Cape Blue Object Survey (Stobie et al. 1997a) is a southern hemisphere survey to discover hot, blue stellar objects brighter than B=18 at galactic latitudes more than 30° from the galactic plane. The main categories of object detected are hot subdwarfs, white dwarfs, blue horizontal branch stars, apparently normal B stars, cataclysmic variables and (stellar-like) active galactic nuclei. Over 50% of the EC Survey comprises hot subdwarfs.

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Amalia Nessa Arlinda, Ayuk Yuliana, Taufiq Khaerudin, Zulfatun Nisa’, Bondan Nugroho, and Diah Agustina Prihastiwi. "Analisis Manajemen Kolaboratif Model Pentahelix Sebagai Strategi Pengelolaan Objek Wisata Pemandian Air Panas Desa Sumberarum Kabupaten Magelang." EKONOMIKA45 : Jurnal Ilmiah Manajemen, Ekonomi Bisnis, Kewirausahaan 11, no. 2 (2024): 371–94. http://dx.doi.org/10.30640/ekonomika45.v11i2.2542.

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This research is motivated by the lack of availability of facilities and infrastructure, competition between managers and lack of human resources in the management of tourism objects. The location of this bathhouse is located in Dimajar Hamlet, Sumberarum Village, Tempuran District, Magelang Regency. The formulation of this research problem is how to analyze the application of the Pentahelix Model Collaborative Management as a Tourism Object Management Strategy in the Hot Springs of Sumberarum Village, Magelang Regency. This research uses the theory of strategic management from Fred R David (2

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Martasari, R. D., S. Pambudi, I. P. Haty, et al. "Geotourism in Mount Pandan and Bledug Kuwu Hotspring as a potential resources for community development." IOP Conference Series: Earth and Environmental Science 1339, no. 1 (2024): 012033. http://dx.doi.org/10.1088/1755-1315/1339/1/012033.

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Abstract Mount Pandan and Bledug Kuwu are popular tourist attractions in the central part of Java Island. Each location has an object that can be analyzed as a geotourism potential, as the manifestation of hot springs. These results indicate that Bledug Kuwu Mud Volcano, Crewek Hot Spring, Banyu Kuning Hot Spring, and Jari Kasinen Hot Spring sites can be geotourism-based tourist objects. Mount Pandan and Bledug Kuwu sites need to be improved in several aspects, especially in terms of infrastructure. Parameters that need to be considered for all objects are conservation values due to disaster r

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Petit, Jean-Marc, Brett Gladman, J. J. Kavelaars, et al. "The Hot Main Kuiper Belt Size Distribution from OSSOS." Astrophysical Journal Letters 947, no. 1 (2023): L4. http://dx.doi.org/10.3847/2041-8213/acc525.

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Abstract Using the absolute detection calibration and abundant detections of the Outer Solar System Origins Survey project, we provide population measurements for the main Kuiper Belt. For absolute magnitude H r < 8.3, there are 30,000 nonresonant main-belt objects, with twice as many hot-component objects than cold, and with total mass of 0.014 M ⊕, only one-seventh of which is in the cold belt (assuming a cold-object albedo about half that of hot-component objects). We show that trans-Neptunian objects with 5.5 < H r < 8.3 (rough diameters 400–100 km) have indistinguishable absolute

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Bratus, Sergey, James Oakley, Ashwin Ramaswamy, Sean W. Smith, and Michael E. Locasto. "Katana." International Journal of Secure Software Engineering 1, no. 3 (2010): 1–17. http://dx.doi.org/10.4018/jsse.2010070101.

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The mechanics of hot patching (the process of upgrading a program while it executes) remain understudied, even though it offers capabilities that act as practical benefits for both consumer and mission-critical systems. A reliable hot patching procedure would serve particularly well by reducing the downtime necessary for critical functionality or security upgrades. However, hot patching also carries the risk—real or perceived—of leaving the system in an inconsistent state, which leads many owners to forgo its benefits as too risky; for systems where availability is critical, this decision may

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Rowe, Jason F., William J. Borucki, David Koch, et al. "KEPLER OBSERVATIONS OF TRANSITING HOT COMPACT OBJECTS." Astrophysical Journal 713, no. 2 (2010): L150—L154. http://dx.doi.org/10.1088/2041-8205/713/2/l150.

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Helmich, F. P., E. F. Van Dishoeck, J. H. Black, and Th De Graauw. "Abundant, hot water toward young stellar objects." Symposium - International Astronomical Union 178 (1997): 397–400. http://dx.doi.org/10.1017/s0074180900009554.

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The large amount of water vapour in the Earth's atmosphere makes it extremely difficult to observe water in interstellar space, except under unusual conditions (e.g., masers). The Short Wavelength Spectrometer (SWS; de Graauw et al. 1996) on board the Infrared Space Observatory (ISO) provides an unique opportunity to study the ro-vibrational fundamental bands of water in absorption against bright infrared continuum sources. Such absorption line data have several advantages over emission observations. For example, only a pencil beam to the infrared source is probed, which minimizes the complica

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Bottinelli, Sandrine, Cecilia Ceccarelli, Roberto Neri, and Jonathan P. Williams. "High-resolution observations of CH3CN in the hot corino of NGC1333-IRAS4A." Proceedings of the International Astronomical Union 4, S251 (2008): 117–18. http://dx.doi.org/10.1017/s1743921308021303.

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AbstractThe formation and evolution of complex organic molecules in the early stages of solar-type protostars (Class 0 objects) is crucial as it sets the stage for the content in pre-biotic molecules of the subsequent proto-planetary nebula. In order to understand the chemistry of these Class 0 objects, it is necessary to perform interferometric observations which allow us to resolve the hot corino, that is the warm, dense inner region of the envelope of a Class 0 object, where the complex organic molecules are located. Such observations exist for only two objects so far, IRAS16293-2422 and NG

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Alford, J. A. J., and J. P. Halpern. "Do Central Compact Objects have Carbon Atmospheres?" Astrophysical Journal 944, no. 1 (2023): 36. http://dx.doi.org/10.3847/1538-4357/acaf55.

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Abstract Only three of the dozen central compact objects (CCOs) in supernova remnants (SNRs) show thermal X-ray pulsations due to nonuniform surface temperature (hot spots). The absence of X-ray pulsations from several unpulsed CCOs has motivated suggestions that they have uniform-temperature carbon atmospheres (UTCAs), which adequately fit their spectra with appropriate neutron star (NS) surface areas. This is in contrast to the two-temperature blackbody or hydrogen atmospheres that also fit well. Here we investigate the applicability of UTCAs to CCOs. We show the following: (i) The phase-ave

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Duckss, Weitter. "White Dwarfs are Small, Fast-Spinning Hot Stars." International Journal of Sciences Volume 8, no. 2019-11 (2019): 23–31. https://doi.org/10.5281/zenodo.3980001.

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In order to determine the density of white dwarfs and other stars I used a database and created several relations, such as mass/volume of different star types, to create comparable dana, the values of rotation, the percentage of the objects orbiting around a central object and the explanation how different speeds of rotation, if unused, influence the irregular derivation of the gravitational results. Some other factors, essential in creating real values in astrophysics, are also analyzed here. The results acquired in such a way reveal a real image, which is impossible to perceive if analysing

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Fan, Jian De, and Jiang Bo Zhu. "Object Tracking Based on Dual-View Stereo System." Advanced Materials Research 850-851 (December 2013): 780–83. http://dx.doi.org/10.4028/www.scientific.net/amr.850-851.780.

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Tracking moving objects in dual-view stereo system is becoming a hot research area in computer vision. To capture the moving objects pixels more accurately, we proposed a new object tracking algorithm which first compute moving objects feature points and then match these points, finally connect the matching feature points and get objects motion trajectories. The algorithm was tested in the video sequences with resolution 640×480 and 768×576 individually. The results show that the algorithm is more robust and the trajectories of the moving objects tracked with our method are more accurate compa

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Song, Jiahao. "Study on Tiny Object Detection." Highlights in Science, Engineering and Technology 1 (June 14, 2022): 1–6. http://dx.doi.org/10.54097/hset.v1i.419.

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Object detection has been one of the most challenging tasks in computer vision and a hot research topic in the world. With the rapid development of in-depth learning technology, researchers have obtained abundant research results in the field of object detection. However, most of the current mainstream object detection methods are based on the modeling of normal scale objects, and the performance of these methods is seriously degraded when they are directly applied to the detection of tiny objects, because the real scene is changing and unknown, and generally there are problems such as object

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Skliarenko, Nataliia, and Olha Romaniuk. "VISUAL AND TACTILE COMMUNICATION “HOT AND COLD” IN DESIGN PRACTICE." Grail of Science, no. 18-19 (September 5, 2022): 414–16. http://dx.doi.org/10.36074/grail-of-science.26.08.2022.67.

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Nowadays it is much harder to impress a modern person or persuade them to do something. Therefore, developers of design objects should constantly examine and study effective methods to influence a potential consumer. For modern people it is no longer interesting to use ordinary objects of the created environment, they want to be real members of the creative process. The participation and interaction in the process of creation provide the tactile communication of people with the object of creation. Certainly, it is the tactile cognition that refers to the higher level of processing and integrat

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Marzo, Asier, and Bruce W. Drinkwater. "Holographic acoustic tweezers." Proceedings of the National Academy of Sciences 116, no. 1 (2018): 84–89. http://dx.doi.org/10.1073/pnas.1813047115.

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Acoustic tweezers use sound radiation forces to manipulate matter without contact. They provide unique characteristics compared with the more established optical tweezers, such as higher trapping forces per unit input power and the ability to manipulate objects from the micrometer to the centimeter scale. They also enable the trapping of a wide range of sample materials in various media. A dramatic advancement in optical tweezers was the development of holographic optical tweezers (HOT) which enabled the independent manipulation of multiple particles leading to applications such as the assembl

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Tang, Yao Wu, and Xiang Liu. "Application of Fuzzy Predictive Control in Grain Drying Coal Burning Hot Air Furnace Temperature Control System." Applied Mechanics and Materials 530-531 (February 2014): 981–84. http://dx.doi.org/10.4028/www.scientific.net/amm.530-531.981.

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Grain drying with chain coalfired hot blast stove for temperature stable and economic operation.Boiler control objects with strong coupling, large delay, large inertia characteristics.Fuzzy control on object for low, fast response and predict advanced features. Design the fuzzy predictive controller for chain coalfired hot blast stove temperature control.The test results show that the fuzzy predictive control system is improved effectively the static precision and dynamic characteristic.Fuzzy predictive control for large delay system has better practicability.

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Large, Nicolas, Lucien Saviot, Jérémie Margueritat, et al. "Acousto-plasmonic Hot Spots in Metallic Nano-Objects." Nano Letters 9, no. 11 (2009): 3732–38. http://dx.doi.org/10.1021/nl901918a.

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Batanov, G. M., N. K. Berezhetskaya, V. A. Kop’ev, I. A. Kossyi, and A. N. Magunov. "Spectral pyrometry of the objects with hot spots." High Temperature 49, no. 5 (2011): 731–35. http://dx.doi.org/10.1134/s0018151x11050026.

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Mitchell, George F., Jean-Pierre Maillard, Mark Allen, Reinhard Beer, and Kenneth Belcourt. "Hot and cold gas toward young stellar objects." Astrophysical Journal 363 (November 1990): 554. http://dx.doi.org/10.1086/169365.

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Chandra, Indriarti. "Pengelolaan Objek Wisata Pemandian Air Panas Cipanas Pandeglang Banten Menurut UU No 10 Tahun 2009 Tentang Kepariwisataan Dalam Mewujudkan Kesejahteraan Masyarakat." Prosiding Seminar Nasional Komunikasi, Administrasi Negara dan Hukum 1, no. 1 (2023): 111–16. http://dx.doi.org/10.30656/senaskah.v1i1.223.

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Indonesia is one of the countries where almost every region has a complete tourist attraction, namely natural beauty, flora, fauna and historical heritage. One of the tourism destinations in Indonesia which has its own potential and attractiveness is Pandeglang Regency, Banten. This study aims to determine the Management of Cipanas Hot Spring Tourism Objects in Developing Tourism Objects According to Law Number 10 of 2009 concerning Tourism and the Impact of Tourism Object Development on the Welfare of the Surrounding Community. In conducting research, the authors use qualitative methods that

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Brickner, Michael S., and Amir Zvuloni. "The Effect of Polarity on Object Recognition in Thermal Images." Proceedings of the Human Factors and Ergonomics Society Annual Meeting 37, no. 1 (1993): 137–41. http://dx.doi.org/10.1177/154193129303700132.

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Thermal imaging (TI) systems, transform the distribution of relative temperatures in a scene into a visible TV image. TIs differ significantly from regular TV images. Most TI systems allow their operators to select preferred polarity which determines the way in which gray shades represent different temperatures. Polarity may be set to either black hot (BH) or white hot (WH). The present experiments were designed to investigate the effects of polarity on object recognition performance in TI and to compare object recognition performance of experts and novices. In the first experiment, twenty fli

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Cauley, P. Wilson. "Discovering the atmospheres of hot Jupiters." Proceedings of the International Astronomical Union 15, S354 (2019): 467–72. http://dx.doi.org/10.1017/s1743921320000198.

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AbstractHot Jupiters are an extraordinary class of exoplanets, orbiting their host stars with periods of hours to a few days. Some of these objects have day-side temperatures approaching photospheric temperatures of late K-type stars. I will give an overview of how we characterize the atmospheres of these fascinating objects and some the more recent exciting results to come from ground and space-based telescopes, as well as what the future holds for detailed characterization of short-period exoplanet atmospheres.

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Kondoj, Telly Hetty Isje, and Vesti L. Sambeka. "Strategies and Models for Development of Hot Water Tourism Objects in Tombasian Village Under Kawangkoan Barat District, Minahasa Regency." Pusaka: Journal of Tourism, Hospitality, Travel and Business Event 4, no. 2 (2022): 188–93. http://dx.doi.org/10.33649/pusaka.v4i2.170.

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Tourism development is sought to be developed in the context of economic improvement, sustainable development and technological development. Geographically, each region has different characteristics with their own uniqueness and advantages. Natural resources that are owned with all its contents, land in all its forms and the sea with all its contents. This potential can be utilized optimally through tourism. Natural resources owned with all their contents and existing potential will be utilized for development purposes. That potential can be an asset through the tourism sector. One of the attr

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Okhotko, N., V. Troianskyi, and O. Bazyey. "PHYSICAL PROPERTIES OF “HOT POPULATION” OBJECTS IN THE KUIPER BELT." Odessa Astronomical Publications 35 (December 14, 2022): 74–76. http://dx.doi.org/10.18524/1810-4215.2022.35.268732.

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Most planetesimals formed at distances of 15 - 30 a.u. were gravitationally ejected from the Solar system as a result of the migration of the giant planets, but a small part remained, captured by Jupiter and the Kuiper belt. As a result, we can now observe such a variety, in terms of physical and dynamic characteristics, in the Trojan asteroids of Jupiter and in the Kuiper belt. Planetesimals captured by the Kuiper Belt are a "hot population" now. The term "hot" does not refer to the temperature of bodies, but characterizes the orbit of objects. ~120,000 objects larger than 100 km. in diameter

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Zhapbasbayev, Uzak, Timur Bekibayev, Gaukhar Ramazanova, and Zhibek Akasheva. "A Digital Twin of Hot Pumping Waxy Oil Through a Main Pipeline." Energies 18, no. 1 (2025): 202. https://doi.org/10.3390/en18010202.

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This article presents a digital twin of hot pumping waxy oil through a main pipeline. Digital copies of the original object data were identified through sensor measurements from SCADA and ECMAS, forming the basis of the SmartTranPro 1.7.1 Software. The mathematical model of the software describes the process of hot pumping waxy oil regarding heat exchange with the environment. The intelligent algorithms of the SmartTranPro 1.7.1 Software were used to determine the actual dependencies of the digital twins of the objects, hydraulic parameters, and heat transfer for the Kassymov–Bolshoi Chagan ho

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Wang, Hongchang, Zhaoyang Jiao, Mingying Sun, Cheng Liu, and Jianqiang Zhu. "High-contrast phase imaging based on nonlinear holographic hot image model." AIP Advances 12, no. 6 (2022): 065315. http://dx.doi.org/10.1063/5.0089116.

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Imaging for weak-phase objects is a challenging issue in the linear imaging process. Here, we demonstrate a high-contrast phase imaging method based on a nonlinear holographic hot image model. Due to the nonlinear Kerr effect, the holographic hot image can transform a weak phase into strong amplitude as a signal amplifier. The phase information is iteratively obtained from the light field distribution of the holographic hot image. The strong signal-to-noise ratio helps improve the imaging contrast. Using a tunable photorefractive crystal, we numerically and experimentally demonstrate the advan

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Hashimotodani, K., K. Hayashida, and T. T. Takeuchi. "ASCA Observation of “Failed Cluster” of Galaxies Candidate, 0806+20." Symposium - International Astronomical Union 188 (1998): 302–3. http://dx.doi.org/10.1017/s0074180900115256.

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The hypothetical object called “failed cluster” of galaxies is described by Tucker et al. (1995, ApJ, 444, 532) as a large cloud of X-ray emitting hot gas without any visible galaxies. They made extensive survey of this type of objects using Einstein IPC database and found only one candidate, 0806+20.

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CASALI, R. H., and D. P. MENEZES. "HOT AND COMPACT STELLAR OBJECTS AND THEIR ADIABATIC INDEX." International Journal of Modern Physics D 19, no. 08n10 (2010): 1477–81. http://dx.doi.org/10.1142/s0218271810017743.

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The adiabatic index of pulsars formed by hadronic or quarkionic matter, with and without trapped neutrinos, is calculated for two values of the entropy per baryon S = 0, 2 kB/baryon. The nonlinear Walecka model1 is used to describe hadronic stars, and the MIT bag model2 to describe quark stars. Particle fractions for each case are obtained and the appearance of particles are shown to coincide with drops in the adiabatic index.

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Wiescher, M., J. Gorres, S. Graff, L. Buchmann, and F. K. Thielemann. "The hot proton-proton chains in low-metallicity objects." Astrophysical Journal 343 (August 1989): 352. http://dx.doi.org/10.1086/167709.

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Prakapenia, Mikalai, and Gregory Vereshchagin. "Pair Creation in Hot Electrosphere of Compact Astrophysical Objects." Astrophysical Journal 963, no. 2 (2024): 149. http://dx.doi.org/10.3847/1538-4357/ad24ee.

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Abstract The mechanism of pair creation in the electrosphere of compact astrophysical objects such as quark stars or neutron stars is revisited, paying attention to evaporation of electrons and acceleration of electrons and positrons, which were previously not addressed in the literature. We perform a series of numerical simulations using the Vlasov–Maxwell equations. The rate of pair creation strongly depends on electric field strength in the electrosphere. Although Pauli blocking is explicitly taken into account, we find no exponential suppression of the pair creation rate at low temperature

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Pluriel, William. "Hot Exoplanetary Atmospheres in 3D." Remote Sensing 15, no. 3 (2023): 635. http://dx.doi.org/10.3390/rs15030635.

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Hot giant exoplanets are very exotic objects with no equivalent in the Solar System that allow us to study the behavior of atmospheres under extreme conditions. Their thermal and chemical day–night dichotomies associated with extreme wind dynamics make them intrinsically 3D objects. Thus, the common 1D assumption, relevant to study colder atmospheres, reaches its limits in order to be able to explain hot and ultra-hot atmospheres and their evolution in a consistent way. In this review, we highlight the importance of these 3D considerations and how they impact transit, eclipse and phase curve o

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Miroshnichenko, Anatoly S., Richard O. Gray, Karen S. Bjorkman, Richard J. Rudy, David K. Lynch, and Alex C. Carciofi. "Properties of the circumstellar dust in galactic FS CMa objects." Proceedings of the International Astronomical Union 6, S272 (2010): 412–13. http://dx.doi.org/10.1017/s1743921311010970.

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AbstractFS CMa objects are a group of hot stars that exhibit the B[e] phenomenon. The group was defined a few years ago on the basis of the formerly known unclassified B[e] stars and newly discovered objects. One of their main features is the presence of hot circumstellar dust whose properties were unknown. We present IR spectra of nearly 20 FS CMa objects obtained with the Spitzer Space Telescope. Dusty features, such as broad silicate bands in emission and narrow bands that are usually explained by PAHs, are detected. The IR fluxes are compared to those detected by IRAS and MSX. Main results

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Van Grootel, V., F. J. Pozuelos, A. Thuillier, et al. "A search for transiting planets around hot subdwarfs." Astronomy & Astrophysics 650 (June 2021): A205. http://dx.doi.org/10.1051/0004-6361/202140381.

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Context. Hot subdwarfs experienced strong mass loss on the red giant branch (RGB) and are now hot and small He-burning objects. These stars constitute excellent opportunities for addressing the question of the evolution of exoplanetary systems directly after the RGB phase of evolution. Aims. In this project we aim to perform a transit survey in all available light curves of hot subdwarfs from space-based telescopes (Kepler, K2, TESS, and CHEOPS) with our custom-made pipeline SHERLOCK in order to determine the occurrence rate of planets around these stars as a function of orbital period and pla

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Hansen, Rickard. "Smoke Stratification in a Mine Drift with Multiple Objects Downstream." Mining Revue 29, no. 1 (2023): 1–18. http://dx.doi.org/10.2478/minrv-2023-0001.

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Abstract The smoke behaviour and smoke stratification of a fire in a mine drift will be one of the decisive factors affecting the risk to mining personnel during a fire. This paper studies the smoke stratification in a mine drift with multiple objects downstream of the fire, at varying distances and number of objects. Data for the study was provided from earlier model-scale fire experiments and CFD modelling was performed for in-depth analysis of specific phenomena. It was found that at considerable downstream distances from the fire, the smoke stratification differences were significant, refl

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Feibelman, Walter A., and Frederick C. Bruhweiler. "Ultraviolet Fe VII absorption lines in planetary nebula nuclei, hot subdwarfs, and hot degenerate objects." Astrophysical Journal 357 (July 1990): 548. http://dx.doi.org/10.1086/168942.

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Zijlstra, A., S. R. Pottasch, P. te Lintel, and C. Bignell. "OH Maser Emission from Young Planetary Nebulae." Symposium - International Astronomical Union 131 (1989): 210. http://dx.doi.org/10.1017/s0074180900138215.

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OH/IR stars are now generally accepted to be progenitors of planetary nebulae. We have carried out a project to try to find objects in the transition phase between OH/IR stars and PN. Transition objects should be characterized by having both continuum radio emission and a 1612 MHz OH maser line. The continuuum emission would indicate that the central star has become hot enough to ionize part of the envelope, while the OH maser indicates that a large part of the envelope is still neutral. Only one such object was known, namely Vy 2-2.

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Jahangiri, Ali, and Mojtaba Biglari. "The stability of vapor film immersed in superfluid helium on the surface of the hot ball." Proceedings of the Institution of Mechanical Engineers, Part E: Journal of Process Mechanical Engineering 230, no. 6 (2016): 433–39. http://dx.doi.org/10.1177/0954408914559571.

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In this article, the evolution of vapor film on the surfaces of hot objects immersed in a cryogenic superfluid helium liquid is considered. It is assumed that at the beginning of the process, a thin film of steam exists on the surface of the object that has a spherical shape. If the heat flux is greater than the critical heat flux, the growth of vapor film will continue, otherwise it will collapse. Survey and analysis of the previously mentioned problem has been done using numerical method and the main onjectives are as follows: (a) study the evolution of the vapor film immersed in superfluid

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Öberg, Karin I., Edith C. Fayolle, John B. Reiter, and Claudia Cyganowski. "Complex molecule formation around massive young stellar objects." Faraday Discuss. 168 (2014): 81–101. http://dx.doi.org/10.1039/c3fd00146f.

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Interstellar complex organic molecules were first identified in the hot inner regions of massive young stellar objects (MYSOs), but have more recently been found in many colder sources, indicating that complex molecules can form at a range of temperatures. However, individually these observations provide limited constraints on how complex molecules form, and whether the same formation pathways dominate in cold, warm and hot environments. To address these questions, we use spatially resolved observations from the Submillimeter Array of three MYSOs together with mostly unresolved literature data

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Evdulov, O. V., A. M. Nasrulaev, and R. Sh Kazumov. "Design of thermoelectric devices for extracting foreign objects from the human body by freezing." Herald of Dagestan State Technical University. Technical Sciences 48, no. 3 (2021): 16–25. http://dx.doi.org/10.21822/2073-6185-2021-48-3-16-25.

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Objectives.The purpose of the article is to consider the designs of thermoelectric devices (TEC) for extracting foreign objects (IO) from the human body by freezing with various options for removing heat from the hot junctions of the thermoelectric module (TEM).Method. Modifications of thermoelectric devices are described for extracting the IO from the human body by freezing it to a special probe. Their technical design differs in the way of heat removal from the TEM hot junctions, for which air heat removal, melting working substances and preliminary cooling of the radiator are used. The basi

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Ulla, A., P. Thejll, S. Vennes, C. S. Hansen-Ruiz, and J. L. Rasilla. "Hot Subdwarfs in Binaries: Multiwavelength Observations and Evolutionary Implications." International Astronomical Union Colloquium 158 (1996): 469–70. http://dx.doi.org/10.1017/s0252921100039452.

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AbstactWe are looking for stellar companions to very hot helium-rich subluminous (sdO) stars by using infrared photometry, optical CCD imaging and spectroscopy. The work is complemented with a comprehensive bibliographic and space-mission databanks search for the objects in our sample (Thejll, Ulla & MacDonald 1995). Companions can be used to indirectly measure the distance to the hot subdwarfs, and give clues about possible binary evolution scenarios. We have therefore gathered and analysed data for 57 hot subdwarfs in a search for IR excesses and companions. 43 of the stars are observed

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Gustya, Wulan Dari. "Analisis Perkembangan Sektor Pariwisata di Kabupaten kerinci." Jurnal Teori dan Riset Administrasi Publik 4, no. 2 (2020): 49–54. http://dx.doi.org/10.24036/jtrap.v4i2.30.

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Abstract This study aims to describe how the development of the tourism sector in Kerinci Regency. This can be seen from the number of tourist objects in Kerinci Regency that have not experienced development, especially from the existing facilities which tend to be less attention by the government. The method used is a qualitative method by interviewing several informants who were met at the tourist attraction site during the research period. The location of this research is a tourist attraction which is the unit of analysis, namely, Semurup Hot Water, Kerinci Lake, Telun Berasap Waterfall, Ar

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BERGER, JACOB. "How Things Seem to Higher-Order Thought Theorists." Dialogue 56, no. 3 (2017): 503–26. http://dx.doi.org/10.1017/s0012217317000440.

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According to David Rosenthal’s higher-order thought (HOT) theory of consciousness, a mental state is conscious just in case one is aware of being in that state via a suitable HOT. Jesse Mulder (2016) recently objects: though HOT theory holds that conscious states are states that it seems to one that one is in, the view seems unable to explain how HOTs engender such seemings. I clarify here how HOT theory can adequately explain the relevant mental appearances, illustrating the explanatory power of HOT theory.

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Nyoman Dwika Ayu Amrita, Agus Wiryadhi Saidi, and Made Mulia Handayani. "Development of Waterfalls and Penikit Hot Springs Tourism Objects in Belok Sidan Village." International Journal of Community Service Learning 6, no. 2 (2022): 185–92. http://dx.doi.org/10.23887/ijcsl.v6i2.40890.

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The attraction of Penikit Waterfall is unique, which is known as a hot and cold waterfall. However, the development of Penikit Waterfall tourism has not sufficiently affected the economy of the local community. The lack of visitors and the lack of information in the wider community about the place is one of the weaknesses of this tourist attraction. In addition, the infrastructure at this tourist attraction is still lacking. For this reason, it is necessary to hold a PKM for the development of Penikit Waterfalls and Hot Springs in Belok Sidan Village, Petang District, Badung Regency. The targe

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Vennes, Stéphane, Péter Németh, and Adela Kawka. "A FEROS Survey of Hot Subdwarf Stars." Open Astronomy 27, no. 1 (2018): 7–13. http://dx.doi.org/10.1515/astro-2018-0005.

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Abstract We have completed a survey of twenty-two ultraviolet-selected hot subdwarfs using the Fiber-fed Extended Range Optical Spectrograph (FEROS) and the 2.2-m telescope at La Silla. The sample includes apparently single objects as well as hot subdwarfs paired with a bright, unresolved companion. The sample was extracted from our GALEX catalogue of hot subdwarf stars. We identified three new short-period systems (P = 3.5 hours to 5 days) and determined the orbital parameters of a long-period (P = 62d.66) sdO plus G III system. This particular system should evolve into a close double degener

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Clarke, Cathie J., and Philip J. Armitage. "The spectroscopic signature of hot Jupiters in FU Orionis objects." Monthly Notices of the Royal Astronomical Society 345, no. 2 (2003): 691–95. http://dx.doi.org/10.1046/j.1365-8711.2003.06983.x.

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Ma, Ding, Zhezhou Yu, JiKun Yu, and Wei Pang. "A Novel Object Tracking Algorithm Based on Compressed Sensing and Entropy of Information." Mathematical Problems in Engineering 2015 (2015): 1–18. http://dx.doi.org/10.1155/2015/628101.

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Object tracking has always been a hot research topic in the field of computer vision; its purpose is to track objects with specific characteristics or representation and estimate the information of objects such as their locations, sizes, and rotation angles in the current frame. Object tracking in complex scenes will usually encounter various sorts of challenges, such as location change, dimension change, illumination change, perception change, and occlusion. This paper proposed a novel object tracking algorithm based on compressed sensing and information entropy to address these challenges. F

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Wadler, Philip. "EDITORIAL: A HOT opportunity." Journal of Functional Programming 7, no. 2 (1997): 127–28. http://dx.doi.org/10.1017/s0956796897002694.

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The Java phenomenon means that programmers that once laughed at garbage collection and strong typing have started to use it daily, and this opens up a wonderful opportunity for the functional programming community.Bob Harper coined the acronym HOT to summarise much of what functional programmers have to offer the world: expertise in languages that are Higher-Order and Typed. Bob argued for a broad interpretation of these terms, so that Higher-Order includes languages where objects contain methods (even though functions are not first-class citizens), and Typed includes both static and dynamic t

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Li, Dongyang. "Research advanced in object detection based on deep learning." Applied and Computational Engineering 5, no. 1 (2023): 603–8. http://dx.doi.org/10.54254/2755-2721/5/20230656.

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In the field of computer vision, identifying specific objects in images and predicting their location and class have long been hot research topics.Algorithms for early object detection rely on traditional handcrafted features, and the speed and precision of their detection cannot meet the needs of real-world applications. Rapid development in convolutional neural networks has accelerated the development of object identification systems based on deep learning.Existing deep learning-based object identification algorithms mostly use two-stage detection and single-stage detection, according to var

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Wei, Peng-Cheng, Fangcheng He, and Jing Li. "Fast detection of moving objects based on sequential images processing." Journal of Intelligent & Fuzzy Systems 39, no. 4 (2020): 5037–44. http://dx.doi.org/10.3233/jifs-179989.

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Nowadays, moving object detection in sequence images has become a hot topic in computer vision research, and has a very wide range of practical applications in many fields of military and daily life. In this paper, fast detection of moving objects in complex background is studied, and fast detection methods for moving objects in static and dynamic scenes are proposed respectively. Firstly, based on image preprocessing, aiming at the difficulty of feature extraction of moving targets in low illumination at night, Gamma change is used to process. Secondly, for the fast detection of moving object

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Nazé, Yaël, and Christian Motch. "Hot stars observed by XMM-Newton." Astronomy & Astrophysics 619 (November 2018): A148. http://dx.doi.org/10.1051/0004-6361/201833842.

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We perform a survey of Oe and Be stars in the X-ray range. To this aim, we cross-correlated XMM-Newton and Chandra catalogs of X-ray sources with a list of Be stars, finding 84 matches in total. Of these, 51 objects had enough counts for a spectral analysis. This paper provides the derived X-ray properties (X-ray luminosities, and whenever possible, hardness ratios, plasma temperatures, and variability assessment) of this largest ever sample of Oe and Be stars. The targets display a wide range in luminosity and hardness. In particular, the significant presence of very bright and hard sources i

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