Relevant bibliographies by topics / Large and giant

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  1. Journal articles
  2. Dissertations / Theses
  3. Books
  4. Book chapters
  5. Conference papers
  6. Reports

Academic literature on the topic 'Large and giant'

Author: Grafiati
Published: 7 June 2025
Last updated: 2 August 2025

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Journal articles on the topic "Large and giant"

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Jurua, Edward, Otto Trust, and Felix Kampindi. "KIC 5110739: A new Red Giant in NGC 6819." Proceedings of the International Astronomical Union 14, S343 (2018): 434–35. http://dx.doi.org/10.1017/s1743921318007998.

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AbstractThe Kepler Input Catalogue (KIC) misclassified a number of red giant stars as sub giants. This could have resulted from the large uncertainties in the KIC surface gravities. This resulted in 1523 stars which were recently classified as red giant stars. The cluster membership of the 1523 red giant stars was determined using age, distance modulus, and variation of colour magnitude with large frequency separation. We found that one star, KIC 5110739, is a member of NGC 6819.
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Kuźmicz, A., B. Czerny, and C. Wildy. "Stellar populations in hosts of giant radio galaxies and their neighbouring galaxies." Astronomy & Astrophysics 624 (April 2019): A91. http://dx.doi.org/10.1051/0004-6361/201834653.

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Context. Giant radio galaxies (with projected linear size of radio structure larger than 0.7 Mpc) are very rare and unusual objects. Only ∼5% of extended radio sources reach such sizes. Understanding of the processes responsible for their large sizes is crucial to further our knowledge about the radio source’s evolution. Aims. We check the hypothesis that giants become extremely large due to the specific history of their host galaxy formation, as well as in the context of the cluster or group of galaxies where they evolve. Therefore we study the star formation histories in their host galaxies
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Musacchio, M., F. Mont'alverne, F. Belzile, C. Riquelme, and A. Tournade. "Large and Giant Aneurysms." Rivista di Neuroradiologia 16, no. 6 (2003): 1253–55. http://dx.doi.org/10.1177/197140090301600658.

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Smiljanic, R., E. Franciosini, A. Bragaglia, et al. "The Gaia-ESO Survey: properties of newly discovered Li-rich giants." Astronomy & Astrophysics 617 (September 2018): A4. http://dx.doi.org/10.1051/0004-6361/201833027.

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Aims. We report 20 new lithium-rich giants discovered within the Gaia-ESO Survey, including the first Li-rich giant with an evolutionary stage confirmed by CoRoT (Convection, Rotation and planetary Transits) data. We present a detailed overview of the properties of these 20 stars. Methods. Atmospheric parameters and abundances were derived in model atmosphere analyses using medium-resolution GIRAFFE or high-resolution UVES (Ultraviolet and Visual Echelle Spectrograph) spectra. These results are part of the fifth internal data release of the Gaia-ESO Survey. The Li abundances were corrected for
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Gehan, C., B. Mosser, E. Michel, R. Samadi, and T. Kallinger. "Core rotation braking on the red giant branch for various mass ranges." Astronomy & Astrophysics 616 (August 2018): A24. http://dx.doi.org/10.1051/0004-6361/201832822.

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Context. Asteroseismology allows us to probe stellar interiors. In the case of red giant stars, conditions in the stellar interior are such as to allow for the existence of mixed modes, consisting in a coupling between gravity waves in the radiative interior and pressure waves in the convective envelope. Mixed modes can thus be used to probe the physical conditions in red giant cores. However, we still need to identify the physical mechanisms that transport angular momentum inside red giants, leading to the slow-down observed for red giant core rotation. Thus large-scale measurements of red gi
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Popowski, Piotr. "The Distance to the Large Magellanic Cloud." International Astronomical Union Colloquium 176 (2000): 203–7. http://dx.doi.org/10.1017/s0252921100057547.

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AbstractI demonstrate that the two unexpected results in the local Universe: anomalous intrinsic (V – I)0 colors of RR Lyrae stars and clump giants in the Galactic center, and very short distances to Magellanic Clouds inferred from clump giants, can be at least partially resolved with a modified coefficient of selective extinction AV/E(V – I). With this modification, I find a new clump-giant distance modulus to the Large Magellanic Cloud, μLMC = 18.27 ± 0.07, which is 0.09 larger than the Udalski (1998b) result. When distance estimates from the red clump, RR Lyrae stars and the eclipsing binar
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Boss, Alan P. "Metallicity and Planet Formation: Models." Proceedings of the International Astronomical Union 5, S265 (2009): 391–98. http://dx.doi.org/10.1017/s1743921310001067.

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AbstractPlanets typically are considerably more metal-rich than even the most metal-rich stars, one indication that planet formation must differ greatly from star formation. There is general agreement that terrestrial planets form by the collisional accumulation of solids composed of heavy elements in the inner regions of protoplanetary disks. Two competing mechanisms exist for the formation of giant planets, core accretion and disk instability, though hybrid combinations are possible as well. In core accretion, a higher metallicity in the protoplanetary disk leads directly to larger core mass
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Ishwara-Chandra, C. H., and D. J. Saikia. "Giant Radio Sources: Evolution and GMRT Observations." Symposium - International Astronomical Union 199 (2002): 199–202. http://dx.doi.org/10.1017/s0074180900168871.

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We study the evolution of giant radio sources and show that they are less luminous than the smaller-sized sources, and are roughly consistent with the evolutionary scenarios where the smaller-sized sources evolve to giants undergoing radiative and expansion losses. Inverse-Compton radiation losses due to the microwave background radiation dominates over the synchrotron losses for giant sources, while for the smaller sources, the latter dominates. We show that giant radio galaxies and quasars are consistent with the unified scheme, and their large sizes are not due to stronger cores. We also pr
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Pawlak, Michał. "Connection between the long secondary period and red giant evolution." Astronomy & Astrophysics 649 (May 2021): A110. http://dx.doi.org/10.1051/0004-6361/202038642.

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Aims. The mechanism behind the long secondary period (LSP) observed in pulsating red giants remains unknown. In this work, I investigate the connection between the red giant branch and the asymptotic giant branch evolution and the appearance of the LSP – a phenomenon that has been observed in a significant proportion of red giants. Methods. For the purposes of this work, I used the OGLE-III sample of the OSARG variables in the Large Magellanic Cloud. I constructed density maps in the period-luminosity as well as color-magnitude planes for the stars showing an LSP and compared them to the remai
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Pasqualin, A. "Storia naturale degli aneurismi “large-giant”." Rivista di Neuroradiologia 16, no. 1 (2003): 135–37. http://dx.doi.org/10.1177/197140090301600117.

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The natural history of large (20–25 mm) and giant (> 25 mm) intracranial aneurysms is still undefined. Most frequently giant aneurysms present with haemorrhage (45% of cases) or symptoms of expanding mass lesion (39% of cases), rarely with ischemic deficits (5% of cases) or epilepsy (2% of cases). Endoluminar thrombosis is present in 48% of large and 73% of giant aneurysms (according to the Italian Cooperative Study of 1988) and constitutes a dynamic process, with possible evolution to: a) sudden mass effect, b) progressive enlargement of the aneurysm, or c) complete spontaneous occlusion;
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Dissertations / Theses on the topic "Large and giant"

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Watson, Shannon M. "Impact of large scale substrate roughness on giant magnetoresistive thin films." W&M ScholarWorks, 2005. https://scholarworks.wm.edu/etd/1539623488.

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This dissertation presents an investigation on the effects of large scale roughness on the properties of giant magnetoresistive multilayers. The large scale roughness (sigmarms > 5 nm) is introduced into giant magnetoresistive thin films through the substrate. Current-in-plane (CIP) and current-perpendicular-to-the-plane (CPP) thin films were deposited by dc magnetron and triode sputtering. All films were characterized for roughness, magnetic and electronic behavior.;Our research on both pseudo spin valves and exchange-biased spin valves shows that long length scale roughness does not have a s
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Garcia, Delia M. "The role of the giant Canada goose (Branta canadensis maxima) cecum in nutrition." Diss., Columbia, Mo. : University of Missouri-Columbia, 2006. http://hdl.handle.net/10355/4354.

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Thesis (Ph.D.)--University of Missouri-Columbia, 2006.<br>The entire dissertation/thesis text is included in the research.pdf file; the official abstract appears in the short.pdf file (which also appears in the research.pdf); a non-technical general description, or public abstract, appears in the public.pdf file. Title from title screen of research.pdf file viewed on (April 25, 2007) Vita. Includes bibliographical references.
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Marshall, Jonathan. "Mass loss from dust-enshrouded Asymptotic Giant Branch stars and red supergiants in the Large Magellanic Cloud." Thesis, Keele University, 2005. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.423432.

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The process of mass-loss from evolved stars is the single largest contributor of matter back into the ISM. Intense mass-loss during the AGB phase of low-intermediate mass stars via a radiatively-driven wind can lead the stars to become enshrouded in an optically-thick layer of dust which condenses out of an extended molecular atmosphere. This thesis attempts to gain further insights into the mass-loss process that is presently poorly understood. We used the Parkes radio telescope to observe dust-enshrouded AGB stars and supergiants in the LMC and SMC, deriving the speed of the superwind from t
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Trabucchi, Michele. "New models of pulsating red giant stars: application to Long-Period Variables in the Large Magellanic Cloud." Doctoral thesis, Università degli studi di Padova, 2018. http://hdl.handle.net/11577/3424579.

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Stars of low and intermediate mass (0.9 ≲ M/M ⊙ ≲ 8) develop an electron-degenerate CO core after the core He-burning phase, and experience the thermally pulsing asymptotic giant branch phase (TP-AGB) as they approach the end of their evolution. Although very short lived, TP-AGB stars are of paramount importance in the study of stellar populations and galaxy evolution. In fact, being intrinsically very bright, they provide a significant contribution to the total luminosity of single stellar populations, and galaxies in general. Most of their radiation is emitted at infrared wavelengths, a spe
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Szentgyorgyi, Andrew, Daniel Baldwin, Stuart Barnes, et al. "The GMT-Consortium Large Earth Finder (G-CLEF): an optical Echelle spectrograph for the Giant Magellan Telescope (GMT)." SPIE-INT SOC OPTICAL ENGINEERING, 2016. http://hdl.handle.net/10150/622810.

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The GMT-Consortium Large Earth Finder (G-CLEF) will be a cross-dispersed, optical band echelle spectrograph to be delivered as the first light scientific instrument for the Giant Magellan Telescope (GMT) in 2022. G-CLEF is vacuumenclosed and fiber-fed to enable precision radial velocity (PRV) measurements, especially for the detection and characterization of low-mass exoplanets orbiting solar-type stars. The passband of G-CLEF is broad, extending from 3500 angstrom to . This passband provides good sensitivity at blue wavelengths for stellar abundance studies and deep red response for observati
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CAMELLINO, DARIO. "IMAGING AND SEROLOGICAL PROFILING OF PATIENTS WITH POLYMYALGIA RHEUMATICA AND GIANT CELL ARTERITIS." Doctoral thesis, Università degli studi di Genova, 2020. http://hdl.handle.net/11567/1010715.

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Background: Polymyalgia rheumatica (PMR) and giant cell arteritis (GCA) are two inflammatory conditions affecting people aged over 50 years. PMR is characterized by pain and stiffness in the shoulder and hip girdles. GCA, a large vessel vasculitis, is the most common form of primary systemic vasculitis. About 40-60% of patients with GCA present with concomitant PMR, and histologic features consistent with GCA can be detected on temporal artery biopsy of about 16% to 21% of patients with PMR. It is still debated whether PMR and GCA are different conditions or represent different clinical manife
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Lowe, Krispian Tom Edward. "Infrared polarimetry and integral field spectroscopy of post-asymptotic giant branch stars." Thesis, University of Hertfordshire, 2008. http://hdl.handle.net/2299/2449.

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In this thesis, I present the properties of IRAS 19306+1407 central source and its sur- rounding circumstellar envelope (CSE), from the analysis of near-infrared (near-IR) polarimetry and integral field spectroscopy (IFS), with supporting archived HST im- ages and sub-millimetre (sub-mm) photometry. This is supported by axi-symmetric light scattering (ALS), axi-symmetric radiative transfer (DART) and molecular hy-drogen (H2) shock models. The polarimetric images show that IRAS 19306+1407 has a dusty torus, which deviates from axisymmetry and exhibits a ‘twist’ feature. The DART and ALS modelli
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Shellnutt, John Gregory. "A-type granites of the Permian Emeishan large igneous province (SW China) implications for the formation of the giant magmatic oxide deposits /." Click to view the E-thesis via HKUTO, 2007. http://sunzi.lib.hku.hk/hkuto/record/B39634498.

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Kim, Dae Wook, James H. Burge, Jonathan M. Davis, et al. "New and improved technology for manufacture of GMT primary mirror segments." SPIE-INT SOC OPTICAL ENGINEERING, 2016. http://hdl.handle.net/10150/622421.

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The Giant Magellan Telescope (GMT) primary mirror consists of seven 8.4 m light-weight honeycomb mirrors that are being manufactured at the Richard F. Caris Mirror Lab (RFCML), University of Arizona. In order to manufacture the largest and most aspheric astronomical mirrors various high precision fabrication technologies have been developed, researched and implemented at the RFCML. The unique 8.4 m (in mirror diameter) capacity fabrication facilities are fully equipped with large optical generator (LOG), large polishing machine (LPM), stressed lap, rigid conformal lap (RC lap) and their proces
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Vieira, Véronique. "Les protéines Discs large, Scribble et Lethal giant larvae : implication dans le développement tumoral dans le modèle murin d'adénocarcinome de l'épithélium pigmentaire TRP1 -TSV40." Paris 7, 2009. http://www.theses.fr/2009PA077008.

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Parmi les tumeurs oculaires les plus fréquentes, le rétinoblastome, une tumeur qui affecte la rétine chez les enfants et le mélanome de la choroïde qui dérive, comme son nome l'indique de la choroïde sont les plus connus. Depuis quelques années, ces deux tumeurs sont largement étudiées et ont mis en évidence des facteurs de prédispositions génétiques. Beaucoup d'entre nous ignorent l'existence d'une autre tumeur oculaire, l'adénocarcinome de l'épithélium pigmentaire de la rétine, qui résulte de la prolifération de l'épithélium pigmentaire de la rétine. Cette tumeur est une tumeur maligne ocula
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Books on the topic "Large and giant"

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McCord, John S. Wyoming giant. Doubleday, 1992.

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Nasser, Dave. Giant George. Ulverscroft, 2012.

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Invisible Giant - Large Print Edition. Independently Published, 2020.

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Ballantyne, Robert Michael. Giant of the North: Large Print. Independently Published, 2019.

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Ballantyne, Robert Michael. Giant of the North: Large Print. Independently Published, 2019.

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Ballantyne, Robert Michael. Giant of the North: Large Print. Independently Published, 2019.

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Ballantyne, Robert Michael. Giant of the North: Large Print. Independently Published, 2019.

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Ballantyne, Robert Michael. Giant of the North: Large Print. Independently Published, 2019.

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Ballantyne, Robert Michael. Giant of the North: Large Print. Independently Published, 2019.

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Ballantyne, Robert Michael. Giant of the North: Large Print. Independently Published, 2019.

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Book chapters on the topic "Large and giant"

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Hauschildt, J., and J. Pulczynski. "The Large Energy Converter Growian." In Taming Giant Projects. Springer Berlin Heidelberg, 2004. http://dx.doi.org/10.1007/978-3-540-24818-7_16.

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Ren, Zeguang. "Large and Giant Aneurysms." In Eight Aneurysms. Springer International Publishing, 2022. http://dx.doi.org/10.1007/978-3-030-97216-5_11.

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Dekel, Avishai, and Erez Braun. "Giant Arcs — Spherical Shells?" In Large Scale Structures of the Universe. Springer Netherlands, 1988. http://dx.doi.org/10.1007/978-94-009-2995-1_149.

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Mao, Guoqiang. "Giant Component in Large Wireless Networks." In Connectivity of Communication Networks. Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-52989-9_4.

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Lynds, Roger, and Vahè Petrosian. "Giant Luminous Arcs in Clusters of Galaxies." In Large Scale Structures of the Universe. Springer Netherlands, 1988. http://dx.doi.org/10.1007/978-94-009-2995-1_62.

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Zhang, Zhiwei. "Multimodality Treatments for Large and Giant Liver Cancers." In Diagnosis and Treatment of Liver Cancer in China. Springer Nature Singapore, 2025. https://doi.org/10.1007/978-981-97-7969-7_12.

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Mellier, Y. "Is the Giant Luminous Arc in A370 a Gravitational Lensing Effect?" In Large Scale Structures of the Universe. Springer Netherlands, 1988. http://dx.doi.org/10.1007/978-94-009-2995-1_61.

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Puri, Ajit S., and Rajsrinivas Parthasarathy. "Balloon-Assisted Catheter Access in Large and Giant Aneurysms." In 100 Interesting Case Studies in Neurointervention: Tips and Tricks. Springer Singapore, 2019. http://dx.doi.org/10.1007/978-981-13-1346-2_23.

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Ramina, Ricardo, Maurício Coelho Neto, Tobias Mattei, Rogério Clemente, and Yvens Barbosa Fernandes. "Surgery of Large and Giant Residual/Recurrent Vestibular Schwannomas." In Samii's Essentials in Neurosurgery. Springer Berlin Heidelberg, 2014. http://dx.doi.org/10.1007/978-3-642-54115-5_25.

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Giannotta, Steven L. "Complication Avoidance for Large and Giant Carotid Ophthalmic Aneurysms." In New Trends in Management of Cerebro-Vascular Malformations. Springer Vienna, 1994. http://dx.doi.org/10.1007/978-3-7091-9330-3_36.

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Conference papers on the topic "Large and giant"

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Ni, Zhiyu, and Chaoyong Yu. "Vibration Control of a Large Space Solar Power Satellite using Giant Magnetostrictive Actuators." In 2024 43rd Chinese Control Conference (CCC). IEEE, 2024. http://dx.doi.org/10.23919/ccc63176.2024.10662324.

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Conan, R., K. Vogiatzis, and H. Fitzpatrick. "Characterization of the Dome Seeing of the Giant Magellan Telescope with Computational Fluid Dynamics Simulations." In Propagation Through and Characterization of Atmospheric and Oceanic Phenomena. Optica Publishing Group, 2024. http://dx.doi.org/10.1364/pcaop.2024.pth1e.1.

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The image quality of ground based telescopes is limited by atmospheric turbulence. The turbulence inside the dome of the telescopes, or dome seeing, accounts for a significant fraction of the image degradation. The Giant Magellan Telescope (GMT) is using extensively computational fluid dynamics simulations, to investigate GMT dome seeing for a large set of environmental conditions.
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Gotthard, Viktor. "Design for Modularity (DFM) Theory and Practice Modular Design of Giant 3D-Printer and 3D-Printed Products." In 10th International Scientific Conference on Advances in Mechanical Engineering. Trans Tech Publications Ltd, 2025. https://doi.org/10.4028/p-bkl5kg.

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Adapting to continuously changing needs and circumstances is a constant challenge for the designers of today. One possible solution to this is a flexible design, which can be effectively accomplished by a system of modular elements. A properly designed modular system can provide sufficient flexibility when configuring the product or equipment for the first time according to current needs. Furthermore, in case of changes in circumstances, the modular system can be easily reconfigured with another, optimized combination of elements according to the new needs. Modular design principles (DFM – Des
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Johns, Matthew W. "Giant Magellan Telescope (GMT)." In Second Backaskog Workshop on Extremely Large Telescopes, edited by Arne L. Ardeberg and Torben Andersen. SPIE, 2004. http://dx.doi.org/10.1117/12.566109.

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Shectman, Stephen A. "Instrumentation for the Giant Magellan Telescope." In Second Backaskog Workshop on Extremely Large Telescopes, edited by Arne L. Ardeberg and Torben Andersen. SPIE, 2004. http://dx.doi.org/10.1117/12.566265.

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Johns, Matt. "The Giant Magellan Telescope (GMT)." In Extremely Large Telescopes: Which Wavelengths? Retirement Symposium for Arne Ardeberg, edited by Torben E. Andersen. SPIE, 2008. http://dx.doi.org/10.1117/12.801254.

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Linardopoulos, Georgios. "Large-spin Expansions of Giant Magnons." In Proceedings of the Corfu Summer Institute 2014. Sissa Medialab, 2015. http://dx.doi.org/10.22323/1.231.0154.

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Whitelock, Patricia. "Large Telescopes and Asymptotic Giant Branch Stars." In STELLAR ASTROPHYSICS WITH THE WORLD'S LARGEST TELESCOPES: First International Workshop on Stellar Astrophysics with the World's Largest Telescopes. AIP, 2005. http://dx.doi.org/10.1063/1.1893340.

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Quirós-Pacheco, Fernando, Antonin Bouchez, Rodolphe Conan, Brian McLeod, and David Schwartz. "The Giant Magellan Telescope Phasing System: algorithms and performance simulations." In Adaptive Optics for Extremely Large Telescopes 5. Instituto de Astrofísica de Canarias (IAC), 2017. http://dx.doi.org/10.26698/ao4elt5.0145.

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Angel, James Roger P., Jon S. Lawrence, and John W. Storey. "Concept for a second Giant Magellan Telescope (GMT) in Antarctica." In Second Backaskog Workshop on Extremely Large Telescopes, edited by Arne L. Ardeberg and Torben Andersen. SPIE, 2004. http://dx.doi.org/10.1117/12.566107.

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Reports on the topic "Large and giant"

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Buchan, K. L., and R. E. Ernst. Paleoproterozoic dyke swarms and large igneous provinces of northern Canada and their use in understanding extension, rifting, and paleocontinental reconstructions. Natural Resources Canada/CMSS/Information Management, 2024. http://dx.doi.org/10.4095/332506.

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Giant mafic dyke swarms and related large igneous provinces play an important role in the understanding of the tectonic evolution of ancient continents and supercontinents. The information available for well dated Paleoproterozoic dyke swarms and large igneous provinces in northern Canada is summarized in this synthesis, with an emphasis on their age, geographic distribution, paleomagnetism, and potential linkages to coeval magmatic events. Their tectonic settings, with a focus on links to rifting and continental breakup, are also discussed. Finally, the use of giant dyke swarms and large igne
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Buchan, K. L., and R. E. Ernst. Giant circumferential and radiating dyke swarms of the High Arctic Large Igneous Province. Natural Resources Canada/ESS/Scientific and Technical Publishing Services, 2017. http://dx.doi.org/10.4095/300702.

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McClure, Michael A., Yitzhak Spiegel, David M. Bird, R. Salomon, and R. H. C. Curtis. Functional Analysis of Root-Knot Nematode Surface Coat Proteins to Develop Rational Targets for Plantibodies. United States Department of Agriculture, 2001. http://dx.doi.org/10.32747/2001.7575284.bard.

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The goal of this research was to provide a better understanding of the interface between root-knot nematodes, Meloidogyne spp., and their host in order to develop rational targets for plantibodies and other novel methods of nematode control directed against the nematode surface coat (SC). Specific objectives were: 1. To produce additional monoclonal SC antibodies for use in Objectives 2, 3, and 4 and as candidates for development of plantibodies. 2. To determine the production and distribution of SC proteins during the infection process. 3. To use biochemical and immunological methods to pertu
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Bradford, John, Caroline Havrilla, Jessica Hartsell, et al. Southeast Utah Group climate and drought adaptation report: Exposure and perennial grass sensitivity. National Park Service, 2022. http://dx.doi.org/10.36967/2293951.

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National Park Service (NPS) managers face growing challenges resulting from the effects of climate change. In particular, as temperatures rise in coming decades, natural resource management in the western United States must cope with expectations for elevated severity and frequency of droughts. These challenges are particularly pronounced for vegetation managers in dryland environments. Developing adaptive strategies requires specific information about the expected magnitude of change in climate and drought conditions as well as insights into how those changes will affect important vegetation
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Salcido, Charles, Patrick Wilson, Justin Tweet, Blake McCan, Clint Boyd, and Vincent Santucci. Theodore Roosevelt National Park: Paleontological resource inventory (public version). National Park Service, 2022. http://dx.doi.org/10.36967/nrr-2293509.

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Theodore Roosevelt National Park (THRO) in western North Dakota was established for its historical connections with President Theodore Roosevelt. It contains not only historical and cultural resources, but abundant natural resources as well. Among these is one of the best geological and paleontological records of the Paleocene Epoch (66 to 56 million years ago) of any park in the National Park System. The Paleocene Epoch is of great scientific interest due to the great mass extinction that occurred at its opening (the Cretaceous–Paleogene extinction event), and the unusual climatic event that
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