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Relevant bibliographies by topics / Accretion phenomena

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Academic literature on the topic 'Accretion phenomena'

Author: Grafiati

Published: 8 June 2024

Last updated: 31 July 2025

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Journal articles on the topic "Accretion phenomena"

1

Bailey, Jeremy. "Accretion Phenomena in Cataclysmic Variables." Publications of the Astronomical Society of Australia 13, no. 1 (1996): 75–80. http://dx.doi.org/10.1017/s1323358000020579.

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AbstractThe processes of accretion onto the white dwarf in a cataclysmic variable are reviewed. These systems provide the most easily observable examples of accretion disks, and enable the structure of the accretion region to be studied in detail. The properties of column accretion onto magnetic cataclysmic variables are also described.

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Walker, Mark. "Accretion-driven nonthermal phenomena." Astrophysical Journal 330 (July 1988): L47. http://dx.doi.org/10.1086/185202.

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KUNCIC, ZDENKA, and GEOFFREY V. BICKNELL. "TOWARDS A NEW STANDARD THEORY FOR ASTROPHYSICAL DISK ACCRETION." Modern Physics Letters A 22, no. 23 (2007): 1685–700. http://dx.doi.org/10.1142/s0217732307024243.

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We briefly review recent developments in black hole accretion disk theory, placing new emphasis on the vital role played by magnetohydrodynamic (MHD) stresses in transporting angular momentum. The apparent universality of accretion-related outflow phenomena is a strong indicator that vertical transport of angular momentum by large-scale MHD torques is important and may even dominate radial transport by small-scale MHD turbulence. This leads to an enhanced overall rate of angular momentum transport and allows accretion of matter to proceed at an interesting rate. Furthermore, we argue that when

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Lee, Umin, and Tod E. Strohmayer. "Thermonuclear Excitation of R-modes in Neutron Stars." International Astronomical Union Colloquium 155 (1995): 445–46. http://dx.doi.org/10.1017/s0252921100037921.

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AbstractNeutron stars display phenomena which result from the burning of accreted nuclear fuel in their surface layers. In addition to producing X-ray bursts and other temporal phenomema, such burning can excite oscillation modes of the neutron star. Here we investigate the stability of R-modes in uniformly rotating neutron stars using nonadiabatic pulsation calculations of steady burning envelopes on accreting neutron stars. We find that the fundamental R-modes are unstable for a large range of accretion rates, and thus might manifest themselves observationally in the power spectra of accreti

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Kim, Hongsu, and Uicheol Jang. "Effect of Radiation Pressure Formed at the Inner Region of the Accretion Disk on the Accretion Flow in the Outer Region." Journal of Astronomy and Space Sciences 40, no. 4 (2023): 247–58. http://dx.doi.org/10.5140/jass.2023.40.4.247.

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Studying the accretion phenomena provides a window into understanding most heavenly bodies, from the birth of stars to active galactic nuclei (AGN). We would adopt the effect of the radiation pressure, which reduces accretion rates ( M ˙ ), on the accretion phenomena. The Shakura-Sunyaev α-disk model of disk accretion is a good candidate theory of advection dominated accretion flow (ADAF). Reduction in the angular velocity leads to the suppression the disk luminosity and surface temperature, essentially indicating the transition of the standard accretion disk model from convection dominated ac

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Yokosawa, M. "Dynamical Evolution of Accretion Flow onto a Black Hole." Symposium - International Astronomical Union 188 (1998): 455–56. http://dx.doi.org/10.1017/s0074180900116006.

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Active galactic nuclei(AGN) produce many type of active phenomena, powerful X-ray emission, UV hump, narrow beam ejection, gamma-ray emission. Energy of these phenomena is thought to be brought out binding energy between a black hole and surrounding matter. What condition around a black hole produces many type of active phenomena? We investigated dynamical evolution of accretion flow onto a black hole by using a general-relativistic, hydrodynamic code which contains a viscosity based on the alpha-model. We find three types of flow's pattern, depending on thickness of accretion disk. In a case

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Ferreira, J. "Accretion-ejection phenomena from young stars." EAS Publications Series 9 (2003): 33. http://dx.doi.org/10.1051/eas:2003083.

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Tanaka, Y. "Outburst Phenomena in X-Ray Binaries." Symposium - International Astronomical Union 151 (1992): 215–24. http://dx.doi.org/10.1017/s0074180900122211.

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Three distinctly different types of outburst phenomenon in X-ray binaries are discussed: (1) the so-called type 1 burst which is a thermonuclear flash of matter accreted on the surface of neutron stars, (2) the so-called type 2 burst which is a burst-like X-ray emission caused by a spasmodic accretion, and (3) the nova-like outburst which is triggered by a sudden commencement of accretion.

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Iijima, T. "Rapid Mass Accretion in the Symbiotic Star AG Dra." International Astronomical Union Colloquium 93 (1987): 759–62. http://dx.doi.org/10.1017/s0252921100105640.

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AbstractThe mass accretion process onto the hot component of AG Dra and its explosive phenomena are discussed. The hot component seems to be a massive white dwarf (M > 1 M⊙). The mass accretion rate is estimated to be about 10−7M⊙/year. Many properties of the explosive phenomena agree with those of mild hydrogen flashes expected from this rapid mass accretion.

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de Gouveia Dal Pino, Elisabete M., and Alex C. Raga. "JD7 -Astrophysical Outflows and Associated Accretion Phenomena." Proceedings of the International Astronomical Union 5, H15 (2009): 235–36. http://dx.doi.org/10.1017/s1743921310009002.

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Highly collimated supersonic jets and outflows are very frequent in several astrophysical environments. They are seen in young stellar objects (YSOs), proto-planetary nebulae, compact objects (like galactic black holes or microquasars, and X-ray binary stars), active galactic nuclei, and are also possibly associated to gamma-ray bursts (GRBs) and to ultra-high energy cosmic rays sources (UHECRs). Despite their different physical scales, all these outflow classes have strong morphological similarities, but questions such as - what physics do they share? - or - can we find a universal mechanism

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Dissertations / Theses on the topic "Accretion phenomena"

1

Hickinbotham, Simon John. "S-Gabor filters for line accretion phenomena." Thesis, University of York, 1999. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.341113.

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Rolfe, Daniel James. "Accretion flow and precession phenomena in cataclysmic variables." Thesis, n.p, 2001. http://library7.open.ac.uk/abstracts/page.php?thesisid=52.

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Smith, Amanda Jane. "Accretion Disc Phenomena in Extreme Mass Ratio Cataclysmic Variables." Thesis, Open University, 2007. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.486254.

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We study a variety of accretion phenomena under the umbrella of extreme mass ratio cataclysmic variables (CVs), employing both observation and numerical simulation. A primary focus is the superhump phenomenon and the underlying eccentric instability and accretion disc precession. We make a detailed examination of the relationship between superhump period excess, f, and system mass ratio, q. We conduct extensive high resolution three-dimensional smoothed particle hydrodynamic (SPH) simulations, improving upon the realism of previous work from both a numerical and physical perspective. We find a

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Symington, Neil H. "Observations and modelling of accretion phenomena in Classical T Tauri stars." Thesis, University of Exeter, 2005. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.421579.

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Finke, Justin David. "Monte Carlo/Fokker-Planck simulations of Accretion Phenomena and Optical Spectra of BL Lacertae Objects." Ohio University / OhioLINK, 2007. http://rave.ohiolink.edu/etdc/view?acc_num=ohiou1181833339.

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De, Jong Sandra. "Accretion processes of radio galaxies at high energies." Phd thesis, Observatoire de Paris, 2013. http://tel.archives-ouvertes.fr/tel-00914365.

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Les NAG (Active galactic nuclei, ou noyaux actifs de galaxie) sont des noyaux galactiques lumineux (L>10^42 erg/s) au centre desquels se trouve un trou noir super massif. Leur énergie lumineuse est libérée lors de l'accrétion sur ce trou noir, soit via un disque d'accrétion, soit via un flux d'accrétion relativement inefficace. Certaines questions, notamment concernant l'origine des jets dans environ 10 % des NAG, n'ont pas encore de réponse. Le Fermi/LAT gamma-ray survey a soulevé une nouvelle question lorsqu'il a détecté un petit groupe de radio galaxies en addition à de nombreux blazars. Le

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Aguilar, Boris. "Experimental study and numerical modeling of accretion phenomena of snow particles at the origin of the formation of accretions on aeronautical structures or civil engineering." Electronic Thesis or Diss., Toulouse, ISAE, 2024. http://www.theses.fr/2024ESAE0003.

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Pour garantir la sécurité des vols dans des conditions de neige, les constructeurs d'aéronefs doivent démontrer que chaque moteur et son système d'admission d'air peuvent fonctionner sur toute la plage de puissance de vol dans des conditions de neigeuse. Cette étude fait partie d'un effort visant à développer des modèles pour l'accumulation de neige.Pour établir le cadre de départ de ce travail sur la modélisation du givrage de la neige, le chapitre 1 est consacré à une revue de la littérature organisée en trois parties. Dans la première partie, les différents processus de création de neige da

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Aimar, Nicolas. "Astrophysique extrême avec GRAVITY : sursauts énergétiques aux abords de l'horizon des événements du trou noir central de la Galaxie." Electronic Thesis or Diss., Université Paris sciences et lettres, 2023. http://www.theses.fr/2023UPSLO006.

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La Voie Lactée, comme a priori toutes les galaxies structurées, abrite en son cœur un trou noir supermassif d'environ 4,3 millions de masses solaires, nommé Sagittarius A* (Sgr A*). Sa taille, liée à sa masse, et sa proximité d'environ 8,3 kpc, en font le trou noir avec la plus grande taille angulaire dans le ciel (~50 μas), ce qui en fait la cible d'études idéales de ce genre d'objets. Les trous noirs sont les objets les plus compacts de l'Univers, avec un champ gravitationnel extrême proche de leur horizon. La description de ces objets et de leur environnement proche nécessite la prise en co

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Kersalé, Evy. "Etude analytique et numérique du développement d'instabilités MHD dans des structures d'accrétion-éjection magnétisées." Phd thesis, Université Joseph Fourier (Grenoble), 2000. http://tel.archives-ouvertes.fr/tel-00724447.

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La première partie de ce travail se propose de définir une nouvelle version du formalisme d'étude des instabilités MHD de pression dans les structures d'accrétion-éjection magnétisées. Ces processus se produisent dans des plasmas confinés magnétiquement et sont très contraignants dans le domaine de la fusion thermonucléaire mais leur influence est peu étudiée dans des contextes astrophysiques. Dans un cadre d'approximation éliminant les ondes magnétosoniques rapides nous avons développé un système d'équations général permettant de s'intéresser à la fois aux modes instables d'interchange et aux

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Tomei, Niccolò. "GRMHD simulations of thick accretion disks in the Event Horizon Telescope era: the role of the mean-field dynamo mechanism." Doctoral thesis, 2022. http://hdl.handle.net/2158/1264722.

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The baryonic matter of the Universe is found almost entirely in the form of plasma, or ionized gas where the moving charges interact with each other through the self-generated currents and the related magnetic fields within a highly material conductive. The energy contained in the plasma in terms of the magnetic field is usually comparable to the kinetic and/or thermal energy of the plasma itself, and many violent observed phenomena are attributable to the sudden release of magnetic energy (e.g. flares and coronal mass ejection in the Sun, gamma ray bursts, gamma flare in magnetars, rel

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Books on the topic "Accretion phenomena"

1

Beskin, Vassily, Gilles Henri, François Menard, Guy Pelletier, and Jean Dalibard, eds. Accretion discs, jets and high energy phenomena in astrophysics. Springer Berlin Heidelberg, 2003. http://dx.doi.org/10.1007/b80353.

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IAU Colloquium (163rd 1996 Port Douglas, Qld.). Accretion phenomena and related outflows: IAU Colloquium 163 : colloquium held in Port Douglas, Queensland, Australia, 15-19 July 1996. Astronomical Society of the Pacific, 1997.

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S, Beskin V., North Atlantic Treaty Organization. Scientific Affairs Division., and Nato Advanced Study Institute (2002 : Les Houches, Haute-Savoie, France)., eds. Accretion discs, jets, and high energy phenomena in astrophysics =: Disques d'accrétion, jets et phénomènes de haute énergie en astrophysique : Ecole d'été de physique des Houches, Session LXXVIII, 29 July-23 August 2002 : Nato Advanced Study Institute, Euro Summer School, Ecole thématique du CNRS. EDP Sciences, 2003.

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(Editor), Vassily Beskin, Gilles Henri (Editor), Francois Menard (Editor), Guy Pelletier (Editor), and Jean Dalibard (Editor), eds. Accretion Disks, Jets and High-Energy Phenomena in Astrophysics (Les Houches - Ecole d'Ete de Physique Theorique). Springer, 2004.

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Pelletier, Guy, Jean Dalibard, Gilles Henri, Vassily Beskin, and Francois Menard. Accretion Disks, Jets and High-Energy Phenomena in Astrophysics: Les Houches Session LXXVIII, July 29 - August 23, 2002. Springer, 2010.

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6

(Editor), Heon-Young Chang, Chang-Hwan Lee (Editor), Mannque Rho (Editor), and Insu Yi (Editor), eds. Explosive Phenomena in Astrophysical Compact Objects: First KIAS Astrophysics Workshop, Seoul, Korea, 24-27 May 2000 (AIP Conference Proceedings / Astronomy and Astrophysics). American Institute of Physics, 2001.

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7

Wickramasinghe, D. T. Accretion Phenomena and Related Outflows: Iau Colloquium 163: Colloquium Held in Port Douglas, Queensland, Australia, 15-19 July 1996 (Astronomical Society of the Pacific Conference Series). Astronomical Society of the Pacific, 1997.

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Tombesi, Francesco. X-ray probe of ultra-fast outflows in active galactic nuclei: An X-ray study of extreme ejection phenomena near accreting supermassive black holes in Seyfert and radio galaxies. LAP Lambert Academic Publishing, 2012.

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Book chapters on the topic "Accretion phenomena"

1

Pringle, J. E. "Accretion Disc Phenomena." In Reviews in Modern Astronomy. Springer Berlin Heidelberg, 1992. http://dx.doi.org/10.1007/978-3-642-77543-7_7.

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Mineshige, S. "Accretion Disk Instabilities." In Nonlinear Phenomena in Stellar Variability. Springer Netherlands, 1993. http://dx.doi.org/10.1007/978-94-011-1062-4_8.

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Kenyon, Scott J. "Accretion Disks and Eruptive Phenomena." In The Origin of Stars and Planetary Systems. Springer Netherlands, 1999. http://dx.doi.org/10.1007/978-94-011-4509-1_18.

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Rebetzky, A., H. Herold, U. Kraus, H. P. Nollert, and H. Ruder. "Accretion Phenomena at Neutron Stars." In Reviews in Modern Astronomy. Springer Berlin Heidelberg, 1990. http://dx.doi.org/10.1007/978-3-642-76238-3_7.

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Schulz, Norbert S. "Accretion Phenomena and Magnetic Activity in YSOs." In The Formation and Early Evolution of Stars. Springer Berlin Heidelberg, 2012. http://dx.doi.org/10.1007/978-3-642-23926-7_8.

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Okuda, T., and S. Mineshige. "Pulsational Instability of Accretion Disks Around Compact Objects." In Nonlinear Phenomena in Stellar Variability. Springer Netherlands, 1993. http://dx.doi.org/10.1007/978-94-011-1062-4_59.

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Heyvaerts, Jean. "Course 1: Accretion and Ejection-Related MHD." In Accretion discs, jets and high energy phenomena in astrophysics. Springer Berlin Heidelberg, 2004. http://dx.doi.org/10.1007/978-3-540-39932-2_1.

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Czerny, Bozena. "Course 9: Accretion around Active Galactic Nuclei." In Accretion discs, jets and high energy phenomena in astrophysics. Springer Berlin Heidelberg, 2004. http://dx.doi.org/10.1007/978-3-540-39932-2_9.

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Honma, F., R. Matsumoto, and S. Kato. "Numerical Simulations of Pulsationally Unstable Accretion Disks Around Supermassive Black Holes." In Nonlinear Phenomena in Stellar Variability. Springer Netherlands, 1993. http://dx.doi.org/10.1007/978-94-011-1062-4_60.

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Kudoh, T., and K. Shibata. "Magnetically Driven Jets From Accretion Disks: Nonsteady And Steady Solutions." In Magnetodynamic Phenomena in the Solar Atmosphere. Springer Netherlands, 1996. http://dx.doi.org/10.1007/978-94-009-0315-9_119.

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Conference papers on the topic "Accretion phenomena"

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Vanbeveren, Dany. "Binaries, cluster dynamics and population studies of stars and stellar phenomena." In INTERACTING BINARIES: Accretion, Evolution, and Outcomes. AIP, 2005. http://dx.doi.org/10.1063/1.2130266.

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Meintjes, Pieter. "Magnetically driven transient phenomena in accretion driven systems: New breakthroughs with meerKAT and CTA?" In Accretion Processes in Cosmic Sources. Sissa Medialab, 2018. http://dx.doi.org/10.22323/1.288.0039.

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Hayashi, Ryosuke, and Makoto Yamamoto. "Numerical Simulation on Ice Accretion Phenomena in Rotor-Stator Interaction Field." In ASME Turbo Expo 2013: Turbine Technical Conference and Exposition. American Society of Mechanical Engineers, 2013. http://dx.doi.org/10.1115/gt2013-95448.

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Ice accretion is a phenomenon where super-cooled water droplets impinge and accrete on a body. On a jet engine, ice accretion disturbs the inlet flow, and separated ice pieces can damage to the turbine component, which leads to the severe performance degradation. We simulated icing phenomena in a fan rotor-stator interaction field [1]. This study mainly focused on the icing property at the rotor blade, because the maximum ice thickness of the rotor blade is about seven times larger than that of the stator vane. Moreover, in the study, the effect of the tip clearance was neglected because of th

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Ferreira, Jonathan. "Theory of magnetized accretion-ejection structures." In High Energy Phenomena in Relativistic Outflows VIII. Sissa Medialab, 2024. http://dx.doi.org/10.22323/1.461.0004.

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Chattopadhyay, Indranil, Mukesh Vyas, and Kuldeep Singh. "Relativistic Jets From Black Hole Accretion Disc." In High Energy Phenomena in Relativistic Outflows VII. Sissa Medialab, 2020. http://dx.doi.org/10.22323/1.354.0007.

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Meintjes, Pieter, and No Co-authors. "Magnetic reconnection and transient phenomena in accretion driven systems." In 4th Annual Conference on High Energy Astrophysics in Southern Africa. Sissa Medialab, 2017. http://dx.doi.org/10.22323/1.275.0032.

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Boula, Stella, Demosthenes Kazanas,, and Apostolos Mastichiadis. "Mhd Accretion Disk Winds And The Blazar Sequence." In High Energy Phenomena in Relativistic Outflows VII. Sissa Medialab, 2020. http://dx.doi.org/10.22323/1.354.0009.

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Tezok, F., M. Brahimi, and I. Paraschivoiu. "Investigation of the physical processes underlying the ice accretion phenomena." In 36th AIAA Aerospace Sciences Meeting and Exhibit. American Institute of Aeronautics and Astronautics, 1998. http://dx.doi.org/10.2514/6.1998-484.

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Furuta, Koharu, and Makoto Yamamoto. "Numerical Simulation on Ice Growth in High-Temperature Environment." In ASME Turbo Expo 2014: Turbine Technical Conference and Exposition. American Society of Mechanical Engineers, 2014. http://dx.doi.org/10.1115/gt2014-25847.

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This paper discusses a fundamental study on icing phenomena in a high-temperature environment. Generally, ice accretion is a phenomenon to form ice layer on a body due to impingement of super-cooled water droplets. In recent years, it is known that ice accretion occurs in the engine core such as the low pressure compressor and the first stage of the high pressure compressor, where the temperature is about 30 degree C. The ice accretion in the engine core is called as “ice crystal accretion”. Some scenarios are given for the ice crystal accretion, but the mechanism has not been sufficiently cla

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Fochi Wang, Yuzhen Lv, Qing Zhang, Zhou You, and Chengrong Li. "Ice accretion on different aluminum cable steel reinforced." In 2010 IEEE Conference on Electrical Insulation and Dielectric Phenomena (CEIDP 2010). IEEE, 2010. http://dx.doi.org/10.1109/ceidp.2010.5723984.

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Reports on the topic "Accretion phenomena"

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Mayas, Magda. Creating with timbre. Norges Musikkhøgskole, 2018. http://dx.doi.org/10.22501/nmh-ar.686088.

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Unfolding processes of timbre and memory in improvisational piano performance This exposition is an introduction to my research and practice as a pianist, in which I unfold processes of timbre and memory in improvised music from a performer’s perspective. Timbre is often understood as a purely sonic perceptual phenomenon. However, this is not in accordance with a site-specific improvisational practice with changing spatial circumstances impacting the listening experience, nor does it take into account the agency of the instrument and objects used or the performer’s movements and gestures. In m

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