Увійти

Готові списки джерел за темами / Stellar object

Зміст

Статті в журналах
Дисертації
Книги
Частини книг
Тези доповідей конференцій
Звіти організацій

Добірка наукової літератури з теми "Stellar object"

Автор: Grafiati

Опубліковано: 28 травня 2022

Оновлено: 31 липня 2025

Оформте джерело за APA, MLA, Chicago, Harvard та іншими стилями

Оберіть тип джерела:

Ознайомтеся зі списками актуальних статей, книг, дисертацій, тез та інших наукових джерел на тему "Stellar object".

Біля кожної праці в переліку літератури доступна кнопка «Додати до бібліографії». Скористайтеся нею – і ми автоматично оформимо бібліографічне посилання на обрану працю в потрібному вам стилі цитування: APA, MLA, «Гарвард», «Чикаго», «Ванкувер» тощо.

Також ви можете завантажити повний текст наукової публікації у форматі «.pdf» та прочитати онлайн анотацію до роботи, якщо відповідні параметри наявні в метаданих.

Статті в журналах з теми "Stellar object"

1

Stobie, R. S., D. Kilkenny, D. O’Donoghue, and A. Chen. "The Edinburgh-Cape Blue Object Survey." International Astronomical Union Colloquium 148 (1995): 280–91. http://dx.doi.org/10.1017/s0252921100022041.

Повний текст джерела

Анотація:

AbstractThe Edinburgh-Cape Blue Object Survey is a major survey to discover blue stellar objects brighter than B ∼ 18 in the southern sky. It covers an area of sky of 10,000 square degrees with |b| > 30° and δ < 0°. The blue stellar objects are selected by automatic techniques from U and B pairs of UK Schmidt Telescope plates scanned with the COSMOS measuring machine. Follow-up photometry and spectroscopy are being obtained with the SAAO telescopes to classify objects brighter than B = 16.5. This paper describes the survey, the techniques used to extract the blue stellar objects, the pho

Стилі APA, Harvard, Vancouver, ISO та ін.

2

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.

Повний текст джерела

Анотація:

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.

Стилі APA, Harvard, Vancouver, ISO та ін.

3

Gautschy, T., H. W. Duerbeck, A. M. Van Genderen, and S. Benetti. "Sakurai’s Object: Constraints from its Variability?" Highlights of Astronomy 11, no. 1 (1998): 360. http://dx.doi.org/10.1017/s1539299600021110.

Повний текст джерела

Анотація:

The peculiar outburst of the star baptized Sakurai’s Object (SO) is a conceivable example of a late He shell flash in a post-AGB object. The new source of nuclear energy forces such objects toward high luminosities and eventually low effective temperatures; they cross the HR diagram in a comparable fashion as FG Sge did in the past - i.e., they move noticeably on the HR diagram on human timescales. From monitoring campaigns of SO during the last year, first estimates of its cooling rate were derived and in particular cyclic light variability was established. We present first results from attem

Стилі APA, Harvard, Vancouver, ISO та ін.

4

Eupen, F., L. Labadie, R. Grellmann, et al. "The GRAVITY young stellar object survey." Astronomy & Astrophysics 648 (April 2021): A37. http://dx.doi.org/10.1051/0004-6361/202039599.

Повний текст джерела

Анотація:

Context. Close young binary stars are unique laboratories for the direct measurement of pre-main-sequence (PMS) stellar masses and their comparison to evolutionary theoretical models. At the same time, a precise knowledge of their orbital parameters when still in the PMS phase offers an excellent opportunity for understanding the influence of dynamical effects on the morphology and lifetime of the circumstellar as well as circumbinary material. Aims. The young T Tauri star WW Cha was recently proposed to be a close binary object with strong infrared and submillimeter excess associated with cir

Стилі APA, Harvard, Vancouver, ISO та ін.

5

Perraut, K., L. Labadie, B. Lazareff, et al. "The GRAVITY Young Stellar Object survey." Astronomy & Astrophysics 632 (November 27, 2019): A53. http://dx.doi.org/10.1051/0004-6361/201936403.

Повний текст джерела

Анотація:

Context. The formation and the evolution of protoplanetary disks are important stages in the lifetime of stars. Terrestrial planets form or migrate within the innermost regions of these protoplanetary disks and so, the processes of disk evolution and planet formation are intrinsically linked. Studies of the dust distribution, composition, and evolution of these regions are crucial to understanding planet formation. Aims. We built a homogeneous observational dataset of Herbig Ae/Be disks with the aim of spatially resolving the sub au-scale region to gain a statistical understanding of their mor

Стилі APA, Harvard, Vancouver, ISO та ін.

6

Caratti o Garatti, A., R. Fedriani, R. Garcia Lopez, et al. "The GRAVITY young stellar object survey." Astronomy & Astrophysics 635 (March 2020): L12. http://dx.doi.org/10.1051/0004-6361/202037583.

Повний текст джерела

Анотація:

Context. The inner regions of the discs of high-mass young stellar objects (HMYSOs) are still poorly known due to the small angular scales and the high visual extinction involved. Aims. We deploy near-infrared spectro-interferometry to probe the inner gaseous disc in HMYSOs and investigate the origin and physical characteristics of the CO bandhead emission (2.3–2.4 μm). Methods. We present the first GRAVITY/VLTI observations at high spectral (ℛ = 4000) and spatial (mas) resolution of the CO overtone transitions in NGC 2024 IRS 2. Results. The continuum emission is resolved in all baselines and

Стилі APA, Harvard, Vancouver, ISO та ін.

7

Koutoulaki, M., R. Garcia Lopez, A. Natta, et al. "The GRAVITY young stellar object survey." Astronomy & Astrophysics 645 (January 2021): A50. http://dx.doi.org/10.1051/0004-6361/202038000.

Повний текст джерела

Анотація:

Context. 51 Oph is a Herbig Ae/Be star that exhibits strong near-infrared CO ro-vibrational emission at 2.3 μm, most likely originating in the innermost regions of a circumstellar disc. Aims. We aim to obtain the physical and geometrical properties of the system by spatially resolving the circumstellar environment of the inner gaseous disc. Methods. We used the second-generation Very Large Telescope Interferometer instrument GRAVITY to spatially resolve the continuum and the CO overtone emission. We obtained data over 12 baselines with the auxiliary telescopes and derive visibilities, and the

Стилі APA, Harvard, Vancouver, ISO та ін.

8

Bouarour, Y. I., K. Perraut, F. Ménard, et al. "The GRAVITY young stellar object survey." Astronomy & Astrophysics 642 (October 2020): A162. http://dx.doi.org/10.1051/0004-6361/202038249.

Повний текст джерела

Анотація:

Context. Studies of the dust distribution, composition, and evolution of protoplanetary disks provide clues for understanding planet formation. However, little is known about the innermost regions of disks where telluric planets are expected to form. Aims. We aim constrain the geometry of the inner disk of the T Tauri star RY Lup by combining spectro-photometric data and interferometric observations in the near-infrared (NIR) collected at the Very Large Telescope Interferometer. We use PIONIER data from the ESO archive and GRAVITY data that were obtained in June 2017 with the four 8m telescope

Стилі APA, Harvard, Vancouver, ISO та ін.

9

Canalizo, Gabriela, and Alan Stockton. "INTERMEDIATE-AGE STELLAR POPULATIONS IN CLASSICAL QUASI-STELLAR OBJECT HOST GALAXIES." Astrophysical Journal 772, no. 2 (2013): 132. http://dx.doi.org/10.1088/0004-637x/772/2/132.

Повний текст джерела

Стилі APA, Harvard, Vancouver, ISO та ін.

10

Bertulani, C. A., M. Naizer, and W. Newton. "Stellar oscillations induced by the passage of a fast stellar object." International Journal of Modern Physics D 23, no. 10 (2014): 1450084. http://dx.doi.org/10.1142/s0218271814500849.

Повний текст джерела

Анотація:

In this paper, we investigate induced oscillations by the gravitational field of a fast stellar object, such as a neutron star or a black-hole in a near miss collision with another star. Nonadiabatic collision conditions may lead to large amplitude oscillations in the star. We show that for a solar-type star a resonant condition can be achieved by a fast moving stellar object with velocity in the range of 100 to 1000 km/s, passing at a distance of a few multiples of the star radius. Although such collisions are rare, they are more frequent than head-on collisions, and their effects could be ob

Стилі APA, Harvard, Vancouver, ISO та ін.

Більше джерел

Дисертації з теми "Stellar object"

1

Tyne, V. H. "A born-again star : the circumstellar environment of Sakurai's object." Thesis, Keele University, 2002. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.251400.

Повний текст джерела

Стилі APA, Harvard, Vancouver, ISO та ін.

2

Kolokoutsas, Konstantinos. "MWC 297 : a case study of a massive young stellar object." Thesis, Imperial College London, 2003. http://hdl.handle.net/10044/1/7661.

Повний текст джерела

Стилі APA, Harvard, Vancouver, ISO та ін.

3

Schworer, Guillaume. "Interferometric observations to analyze circumstellar environments and planetary formation." Thesis, The University of Sydney, 2016. http://hdl.handle.net/2123/16008.

Повний текст джерела

Анотація:

Protoplanetary disks have a rich structure, with different physics playing a role in different regions of the disk. They are under constant evolution, due to a combination of various physical and chemical processes, e.g., accretion, photo-evaporation, gas-dust interactions, grain growth, and the interaction with protoplanets. The dynamic ranges involved span orders of magnitudes on spatial scales, orbital times, temperatures, and dust- or gas-densities. The extreme dynamic ranges involved in the structure and composition of these objects mean that very different observational techniques have t

Стилі APA, Harvard, Vancouver, ISO та ін.

4

Schworer, Guillaume. "Interferometric observations to analyze circumstellar environments and planetary formation." Thesis, Paris Sciences et Lettres (ComUE), 2016. http://www.theses.fr/2016PSLEO018/document.

Повний текст джерела

Анотація:

La poussière et le gaz qui entourent beaucoup d'étoiles jeunes sont d'un intérêt critique pour comprendre la formation planétaire ; ils représentent les conditions initiale de la formation planétaire. Les disques proto-planétaire ont une structure riche, avec différents processus physiques à l'oeuvre dans différentes régions du disque. Les grandeurs en jeu s'étalent sur 2 à 5 ordres de grandeur en échelles spatiales, période orbitale, températures, et bien plus en ce qui concerne la densité de gaz et poussière. Les variations extrêmes de ces paramètres clés impliqués dans la structure et la co

Стилі APA, Harvard, Vancouver, ISO та ін.

5

Ziosi, Brunetto Marco. "The impact of stellar evolution and dynamics on the formation of compact-object binaries." Doctoral thesis, Università degli studi di Padova, 2015. http://hdl.handle.net/11577/3424212.

Повний текст джерела

Анотація:

The aim of this work is to study the formation and evolution of double compact-object binaries (DCOBs, i.e. black hole-black hole, black hole-neutron star and neutron star-neutron star binaries) in young (< 100 Myr) dense (>~ 10^3 star/pc^3) star clusters (YSCs). DCOBs, when merging, are expected to be powerful sources of gravitational waves (GWs) observable by Virgo and LIGO detectors. Best merger candidates (BMCs), i.e. those sources with a chance to be observed, have a coalescence timescale shorter than one Hubble time (t_H) and produce a signal strong enough (strain >~ 10^-21) to be

Стилі APA, Harvard, Vancouver, ISO та ін.

6

Ігнатенко, Вікторія Михайлівна, Виктория Михайловна Игнатенко, Viktoriia Mykhailivna Ihnatenko та А. І. Курман. "Дослідження зоряних об'єктів". Thesis, Видавництво СумДУ, 2011. http://essuir.sumdu.edu.ua/handle/123456789/14075.

Повний текст джерела

Стилі APA, Harvard, Vancouver, ISO та ін.

7

Angus, Ruth. "Stellar ages and stellar rotation." Thesis, University of Oxford, 2016. https://ora.ox.ac.uk/objects/uuid:07f78624-adfe-4775-9d3e-dbc63636156a.

Повний текст джерела

Анотація:

Stellar ages will play a big role in the next generation of astronomy. Useful to exoplaneteers and galactic archaeologists alike, this relatively under-exploited stellar property is currently limited by the precision of dating techniques. The work presented in this thesis contributes incrementally to a greater understanding of rotation period decay in Main Sequence (MS) stars as a proxy for stellar age. Inferring stellar ages from rotation periods, 'gyrochronology', is the only dating method with the potential to provide ages for stars on the hundreds-of-thousands scale. Unfortunately however,

Стилі APA, Harvard, Vancouver, ISO та ін.

8

Wilkins, T. N. "Herbig-Haro objects and stellar jets." Thesis, University of Manchester, 1988. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.234247.

Повний текст джерела

Стилі APA, Harvard, Vancouver, ISO та ін.

9

Holloway, Richard Peter. "Infrared spectropolarimetry of young stellar objects." Thesis, University of Hertfordshire, 2003. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.275217.

Повний текст джерела

Стилі APA, Harvard, Vancouver, ISO та ін.

10

Price, Nigel Mark. "Dynamical interactions between young stellar objects." Thesis, University of Cambridge, 1995. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.387738.

Повний текст джерела

Стилі APA, Harvard, Vancouver, ISO та ін.

Більше джерел

Книги з теми "Stellar object"

1

Manner, Boris. Dieses obskure Objekt der Kunst: That obscure object of art. Kunsthistorisches Museum Wien, 2008.

Знайти повний текст джерела

Стилі APA, Harvard, Vancouver, ISO та ін.

2

Fernandes, A. J. L., P. J. V. Garcia, and J. J. G. Lima, eds. Jets in Young Stellar Objects. Springer Netherlands, 2003. http://dx.doi.org/10.1007/978-94-007-0999-7.

Повний текст джерела

Стилі APA, Harvard, Vancouver, ISO та ін.

3

S, Miller Joseph, and Summer Workshop in Astronomy & Astrophysics (7th : 1984 : Santa Cruz, Calif.), eds. Astrophysics of active galaxies and quasi-stellar objects. University Science Books, 1985.

Знайти повний текст джерела

Стилі APA, Harvard, Vancouver, ISO та ін.

4

Szczerba, Ryszard, and Sławomir K. Górny, eds. Post-AGB Objects as a Phase of Stellar Evolution. Springer Netherlands, 2001. http://dx.doi.org/10.1007/978-94-015-9688-6.

Повний текст джерела

Стилі APA, Harvard, Vancouver, ISO та ін.

5

C, Begelman Mitchell, and United States. National Aeronautics and Space Administration., eds. Radiation pressure-driven magnetic disk winds in broad absorption line quasi-stellar objects. National Aeronautics and Space Administration, 1995.

Знайти повний текст джерела

Стилі APA, Harvard, Vancouver, ISO та ін.

6

C, Begelman Mitchell, and United States. National Aeronautics and Space Administration., eds. Radiation pressure-driven magnetic disk winds in broad absorption line quasi-stellar objects. National Aeronautics and Space Administration, 1995.

Знайти повний текст джерела

Стилі APA, Harvard, Vancouver, ISO та ін.

7

R, Szczerba, and Górny S. K, eds. Post-AGB objects as a phase of stellar evolution: Proceedings of the Toruń workshop held July 5-7, 2000. Kluwer Academic Publishers, 2001.

Знайти повний текст джерела

Стилі APA, Harvard, Vancouver, ISO та ін.

8

Hartmann, Lee. [Theoretical studies of the outer envelopes of young stellar objects]: [semiannual progress report no. 16, 1 Oct. 1983 - 31 Dec. 1991]. Smithsonian Astrophysical Laboratory, 1992.

Знайти повний текст джерела

Стилі APA, Harvard, Vancouver, ISO та ін.

9

Buchholz, Ralf. Eingedrückte Streifen: "... eine wohlthuende Unterbrechung kahler Stellen" : ein Gestaltungsmittel auf Holzoberflächen zwischen 1450 und 1600 in Mitteleuropa. Bubenverlag, 2018.

Знайти повний текст джерела

Стилі APA, Harvard, Vancouver, ISO та ін.

10

Veronika, Darius, Jockel Nils, Suhl Vivian J, and Museum für Kunst und Gewerbe Hamburg., eds. Design Dasein: Ausgewählte Objekte zum Sitzen, Stellen und Leben : Museum für Kunst und Gewerbe Hamburg. Das Museum, 1987.

Знайти повний текст джерела

Стилі APA, Harvard, Vancouver, ISO та ін.

Більше джерел

Частини книг з теми "Stellar object"

1

Jangid, Ankita, and K. K. Venkataratnam. "Relativistic Modelling for Anisotropic Stellar Object." In Advances in Mathematical Modelling, Applied Analysis and Computation. Springer Nature Switzerland, 2024. http://dx.doi.org/10.1007/978-3-031-56304-1_3.

Повний текст джерела

Стилі APA, Harvard, Vancouver, ISO та ін.

2

Ray, T. P., T. Bührke, and R. Mundt. "Pinch Instabilities in Young Stellar Object Jets." In Formation and Evolution of Low Mass Stars. Springer Netherlands, 1988. http://dx.doi.org/10.1007/978-94-009-3037-7_17.

Повний текст джерела

Стилі APA, Harvard, Vancouver, ISO та ін.

3

Depagne, Éric. "4MOST: 4m Multi Object Spectroscopic Telescope." In Asteroseismology of Stellar Populations in the Milky Way. Springer International Publishing, 2014. http://dx.doi.org/10.1007/978-3-319-10993-0_17.

Повний текст джерела

Стилі APA, Harvard, Vancouver, ISO та ін.

4

Forbrich, J., K. Schreyer, B. Posselt, R. Klein, and Th Henning. "UYSO 1 — An Extremely Young Massive Stellar Object." In Springer Proceedings in Physics. Springer Berlin Heidelberg, 1997. http://dx.doi.org/10.1007/978-3-642-18902-9_113.

Повний текст джерела

Стилі APA, Harvard, Vancouver, ISO та ін.

5

Petr-Gotzens, M. G., J. G. Cuby, M. F. Sterzik, P. Schilke, and A. Walsh. "VLT Observations of the Young Stellar Object TMR-1." In The Origins of Stars and Planets: The VLT View. Springer Berlin Heidelberg, 2002. http://dx.doi.org/10.1007/978-3-662-40277-1_51.

Повний текст джерела

Стилі APA, Harvard, Vancouver, ISO та ін.

6

Sauty, Christophe, Noemie Globus, Zakaria Meliani, Kanaris Tsinganos, Nektarios Vlahakis, and Edo Trussoni. "On the Effect of Stellar Wind Braking onto the Central Object." In Protostellar Jets in Context. Springer Berlin Heidelberg, 2009. http://dx.doi.org/10.1007/978-3-642-00576-3_21.

Повний текст джерела

Стилі APA, Harvard, Vancouver, ISO та ін.

7

Duari, D., P. Dasgupta, and J. V. Narlikar. "Peaks And Periodicities In The Redshift Distribution Of Quasi-Stellar Object." In Examining the Big Bang and Diffuse Background Radiations. Springer Netherlands, 1996. http://dx.doi.org/10.1007/978-94-009-0145-2_80.

Повний текст джерела

Стилі APA, Harvard, Vancouver, ISO та ін.

8

Eislöffel, Jochen, and Reinhard Mundt. "Proper Motion Measurements in Various Young Stellar Object Jets in Taurus." In Shocks in Astrophysics. Springer Netherlands, 1995. http://dx.doi.org/10.1007/978-94-009-1624-1_7.

Повний текст джерела

Стилі APA, Harvard, Vancouver, ISO та ін.

9

Goddi, C., L. Moscadelli, W. Alef, and J. Brand. "EVN Observations of H2O Masers Towards the High-Mass Young Stellar Object in AFGL 5142." In Dense Molecular Gas Around Protostars and in Galactic Nuclei. Springer Netherlands, 2005. http://dx.doi.org/10.1007/1-4020-3831-3_9.

Повний текст джерела

Стилі APA, Harvard, Vancouver, ISO та ін.

10

Hanslmeier, Arnold, and Roman Brajša. "Rotational Properties of Compact Objects." In Stellar Rotation. Springer Nature Singapore, 2024. http://dx.doi.org/10.1007/978-981-97-3365-1_7.

Повний текст джерела

Стилі APA, Harvard, Vancouver, ISO та ін.

Тези доповідей конференцій з теми "Stellar object"

1

Perot, Etienne, and Frédérick Viaud. "GYSELE : An Attitude Estimation and Non-Stellar Object Tracking System." In IAF Astrodynamics Symposium, Held at the 75th International Astronautical Congress (IAC 2024). International Astronautical Federation (IAF), 2024. https://doi.org/10.52202/078368-0009.

Повний текст джерела

Стилі APA, Harvard, Vancouver, ISO та ін.

2

Riber, Adrián García, and Francisco Serradilla. "Corot Light Curve Ambsonics/Binaural Sonification." In ICAD 2024: The 29th International Conference on Auditory Display. International Community for Auditory Display, 2024. http://dx.doi.org/10.21785/icad2024.010.

Повний текст джерела

Анотація:

This work describes the design and implementation strategies used in the development of an interactive spatialized multimodal display for the exploration of the light curves from the Convection, Rotation and planetary Transits (CoRoT) archive from the Institut d’Astrophysique Spatiale (IAS). The application displays the representations in a user-selectable Ambisonics or Binaural configuration based on the actual coordinates of the objects. Each sonification is based on a symbolic spectral-type to musical-note mapping strategy, providing musical aesthetics and auditory spectral differentiation

Стилі APA, Harvard, Vancouver, ISO та ін.

3

Paxman, Richard G., Timothy J. Schulz, and James R. Fienup. "Phase-Diverse Speckle Interferometry." In Signal Recovery and Synthesis. Optica Publishing Group, 1992. http://dx.doi.org/10.1364/srs.1992.tua2.

Повний текст джерела

Анотація:

Imaging extended objects through atmospheric turbulence can be accomplished with stellar speckle interferometry, which requires the collection of many image frames of the same object. The exposure time for each frame must be short enough (≈ 10 msec) that the evolving atmosphere can be regarded as frozen during the exposure. Current stellar speckle interferometric approachs, including Labeyrie’s method, Knox-Thompson, and triple correlation, perform an averaging of the data in the process of individually estimating the Fourier modulus or the Fourier phase of the object. The final estimated obje

Стилі APA, Harvard, Vancouver, ISO та ін.

4

Dmitrienko, N. S., P. A. Boley, and S. Y. Melnikov. "INVESTIGATIONS OF THE YOUNG STELLAR OBJECT TH 28." In 48-th International student's conferences "Physics of Space". Ural University Press, 2020. http://dx.doi.org/10.15826/b978-5-7996-2935-9.09.

Повний текст джерела

Стилі APA, Harvard, Vancouver, ISO та ін.

5

Aitken, G. J. M., R. Johnson, and J. Meng. "Photon-Limited Performance of Three Stellar Speckle Image Reconstruction Algorithms." In Quantum-Limited Imaging and Image Processing. Optica Publishing Group, 1989. http://dx.doi.org/10.1364/qlip.1989.tua3.

Повний текст джерела

Анотація:

Atmospheric turbulence limits the resolution of conventional astronomical observations through large ground-based telescopes to about 1". Recently, sub-arcsecond resolution has been achieved by estimating the complex spatial spectrum of a stellar object from a sequence of short-exposure images called specklegrams. Speckle interferometry (SI) gives the diffraction-limited modulus [1]. Phase-measuring processes are the Knox-Thompson (KT) [2], the closely related Phase-Gradient (PG) [3] and the Triple-Correlation (TC) [4] algorithms. Because of the narrow bandwidth, Δλ ≈ 10 nm, and short-exposure

Стилі APA, Harvard, Vancouver, ISO та ін.

6

Riis, T., J. L. Jorgensen, and M. Betto. "Operations of a non-stellar object tracker in space." In 1999 IEEE Aerospace Conference. Proceedings (Cat. No.99TH8403). IEEE, 1999. http://dx.doi.org/10.1109/aero.1999.793150.

Повний текст джерела

Стилі APA, Harvard, Vancouver, ISO та ін.

7

Gatilova, D., E. G. Larionova, T. S. Grishina, and G. A. Borman. "Standardization of the Lacertae 3C 371." In 51-st All-Russian with international participation student scientific conference "Physics of Space". Ural University Press, 2024. http://dx.doi.org/10.15826/b978-5-7996-3848-1.13.

Повний текст джерела

Анотація:

The work is devoted to determining the stellar magnitudes of candidates for comparison stars for Lacertae 3C 371 in the standard Johnson-Cousins photometric system. The brightness of 12 stars located within 10' distance from the object was measured. The obtained standard stellar magnitudes in bands B, V, Rc, Ic are given. The selected stars have a wide range of color indicators and can be used to study the photometric variability of object 3C 371 in various phases of its activity.

Стилі APA, Harvard, Vancouver, ISO та ін.

8

Baba, Naoshi, Susumu Kuwamura, Noriaki Miura, and Yuji Norimoto. "Speckle Spectroscopy under Atmospheric Turbulence." In Advances in Optical Imaging and Photon Migration. Optica Publishing Group, 2022. http://dx.doi.org/10.1364/aoipm.1994.wpl.60.

Повний текст джерела

Анотація:

A method for speckle spectroscopy under atmospheric turbulence is described. A stellar speckle image and its dispersed speckle image are observed simultaneously. An object is reconstructed from speckle images, and its spectrum is reconstructed from dispersed speckle images referring to their speckle images. The shift-and-add reconstruction method is discussed in comparison with ballistic light imaging. Several observational results show that stellar spectroscopy with high-spatial resolution is feasible even under atmospheric turbulence.

Стилі APA, Harvard, Vancouver, ISO та ін.

9

Meng, J., and G. J. M. Aitken. "Triple correlation reconstruction of photon-limited stellar images." In OSA Annual Meeting. Optica Publishing Group, 1989. http://dx.doi.org/10.1364/oam.1989.thm1.

Повний текст джерела

Анотація:

The triple correlation (TC) algorithm, or bispectrum method, has proved to be a robust and reliable technique for recovering atmospherically perturbed, stellar spatial spectra up to the diffraction limit of large telescopes. At very low light levels where the number of detected photons per image is of the order of 102, images are recorded as lists of photon addresses, and computational efficiency can be achieved by exploiting the binary nature of the photon events. In this paper we report experience with the photon address, subplane (PAS) implementation of the TC algorithm. Because the varianc

Стилі APA, Harvard, Vancouver, ISO та ін.

10

Casalbuoni, Roberto. "On the Ground State of QCD inside a Compact Stellar Object." In Proceedings of the 2006 International Workshop. WORLD SCIENTIFIC, 2008. http://dx.doi.org/10.1142/9789812790750_0012.

Повний текст джерела

Стилі APA, Harvard, Vancouver, ISO та ін.

Звіти організацій з теми "Stellar object"

1

Wüthrich, Annik. The Copenhagen Wooden Stela AAd6 from the National Museum of Denmark: An unusual Testimony of the 22nd Dynasty. Verlag der Österreichischen Akademie der Wissenschaften, 2021. http://dx.doi.org/10.1553/erc_stg_757951_the_copenhagen_wooden_stela_aad6_from_the_national_museum_of_denmark_an_unusual_testimony_of_the_22nd_dynasty.

Повний текст джерела

Анотація:

The subject of this article is a wooden stela (AAd6) kept in the National Museum of Denmark in Copenhagen. By iconographical and typological criteria, this object is datable to the 22nd Dynasty and probably comes from the Theban area. The stela displays several particularities, among others, one of the longest genealogies preserved on this object type. Alongside a careful investigation of the different iconographical elements and a new translation of the text, this contribution looks into the onomastic and the prosopographical material, examining different titles such as “ḥnk-nw.w-priest in so

Стилі APA, Harvard, Vancouver, ISO та ін.

2

R. I. EPSTEIN, V. BAILEY, and ET AL. LOW LUMINOSITY COMPACT STELLAR OBJECTS AND THE SIZE OF THE UNIVERSE. Office of Scientific and Technical Information (OSTI), 2000. http://dx.doi.org/10.2172/764697.

Повний текст джерела

Стилі APA, Harvard, Vancouver, ISO та ін.

3

Ziegler, Britta, and Sylvia Crumbach. Der ArcheoKoffer - mittelalterliches Leben im böhmisch-bayerischen Grenzgebiet : Mitmachangebot 1 für Schulklassen : den Geschichtspark Bärnau-Tachov im Klassenzimmer erleben. Otto-Friedrich-Universität, 2024. http://dx.doi.org/10.20378/irb-94659.

Повний текст джерела

Анотація:

Der Lehrstuhl für Archäologie des Mittelalters und der Neuzeit ist eng verflochten mit dem 2011 eröffneten Geschichtspark Bärnau-Tachov im östlichen Landkreis Tirschenreuth, in der Oberpfalz. Die Anlage ist mit einer Fläche von fast 11 ha und über 30 authentisch nachgebauten Gebäuden das größte mittelalterliche archäologische Freilichtmuseum Süddeutschlands und stellt das Alltagsleben in der Bavaria Slavica vom 8./9. bis zum 14. Jahrhundert dar. Der Lehrstuhl für Archäologie des Mittelalters und der Neuzeit, der bereits seit 2010 im wissenschaftlichen Beirat des Geschichtsparks engagiert ist,

Стилі APA, Harvard, Vancouver, ISO та ін.

4

Meyer, Erik. Night Skies Data Report: Photometric Assessment of Night Sky Quality at Dinosaur National Monument. National Park Service, 2025. https://doi.org/10.36967/2314522.

Повний текст джерела

Анотація:

This report characterizes night sky conditions in Dinosaur National Monument (DINO) using measurements made in the park unit and models of regional conditions based on satellite data. Calibrated night sky imagery was obtained to characterize the night sky at 4 sites. These ground-based observations were collected on 4 nights from July 15, 2009 to June 13, 2012. Satellite data from 2024 were used to create a map of predicted night sky conditions in and around the park. The sky overhead remains excellent with an average zenith brightness of 21.99 mag/arcsec2. We estimate more than 96.90% naked e

Стилі APA, Harvard, Vancouver, ISO та ін.

5

Hrynick, Tabitha, and Megan Schmidt-Sane. Note d’Orientation sur l’Engagement Communautaire Concernant la Riposte Contre la Flambée Epidémique de Choléra dans la Région Afrique de l’Est et Australe. Institute of Development Studies, 2023. http://dx.doi.org/10.19088/sshap.2023.008.

Повний текст джерела

Анотація:

Les flambées épidémiques de choléra s’intensifient dans la région Afrique de l’Est et australe (ESAR) depuis janvier 2023, avec une transmission généralisée et étendue au Malawi et au Mozambique, ainsi que des flambées épidémiques signalées en Tanzanie, en Afrique du Sud, au Zimbabwe, au Burundi et en Zambie.1 Il existe un risque de propagation accrue causée par les effets du cyclone Freddy, qui a frappé Madagascar, le Malawi et le Mozambique en mars 2023. Les flambées épidémiques se poursuivent en Somalie, en Éthiopie, au Kenya et au Soudan du Sud, où les pays sont confrontés à la sécheresse

Стилі APA, Harvard, Vancouver, ISO та ін.

Ми пропонуємо знижки на всі преміум-плани для авторів, чиї праці увійшли до тематичних добірок літератури. Зв'яжіться з нами, щоб отримати унікальний промокод!