Gotowa bibliografia na temat „Accretion phenomena”
Utwórz poprawne odniesienie w stylach APA, MLA, Chicago, Harvard i wielu innych
Spis treści
Zobacz listy aktualnych artykułów, książek, rozpraw, streszczeń i innych źródeł naukowych na temat „Accretion phenomena”.
Przycisk „Dodaj do bibliografii” jest dostępny obok każdej pracy w bibliografii. Użyj go – a my automatycznie utworzymy odniesienie bibliograficzne do wybranej pracy w stylu cytowania, którego potrzebujesz: APA, MLA, Harvard, Chicago, Vancouver itp.
Możesz również pobrać pełny tekst publikacji naukowej w formacie „.pdf” i przeczytać adnotację do pracy online, jeśli odpowiednie parametry są dostępne w metadanych.
Artykuły w czasopismach na temat "Accretion phenomena"
Walker, Mark. "Accretion-driven nonthermal phenomena". Astrophysical Journal 330 (lipiec 1988): L47. http://dx.doi.org/10.1086/185202.
Pełny tekst źródłaBailey, Jeremy. "Accretion Phenomena in Cataclysmic Variables". Publications of the Astronomical Society of Australia 13, nr 1 (styczeń 1996): 75–80. http://dx.doi.org/10.1017/s1323358000020579.
Pełny tekst źródłaKUNCIC, ZDENKA, i GEOFFREY V. BICKNELL. "TOWARDS A NEW STANDARD THEORY FOR ASTROPHYSICAL DISK ACCRETION". Modern Physics Letters A 22, nr 23 (30.07.2007): 1685–700. http://dx.doi.org/10.1142/s0217732307024243.
Pełny tekst źródłaLee, Umin, i 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.
Pełny tekst źródłaFerreira, J. "Accretion-ejection phenomena from young stars". EAS Publications Series 9 (2003): 33. http://dx.doi.org/10.1051/eas:2003083.
Pełny tekst źródłaKim, Hongsu, i 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, nr 4 (grudzień 2023): 247–58. http://dx.doi.org/10.5140/jass.2023.40.4.247.
Pełny tekst źródłaYokosawa, 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.
Pełny tekst źródłaTanaka, Y. "Outburst Phenomena in X-Ray Binaries". Symposium - International Astronomical Union 151 (1992): 215–24. http://dx.doi.org/10.1017/s0074180900122211.
Pełny tekst źródłaIijima, 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.
Pełny tekst źródłade Gouveia Dal Pino, Elisabete M., i Alex C. Raga. "JD7 -Astrophysical Outflows and Associated Accretion Phenomena". Proceedings of the International Astronomical Union 5, H15 (listopad 2009): 235–36. http://dx.doi.org/10.1017/s1743921310009002.
Pełny tekst źródłaRozprawy doktorskie na temat "Accretion phenomena"
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.
Pełny tekst źródłaRolfe, Daniel James. "Accretion flow and precession phenomena in cataclysmic variables". Thesis, n.p, 2001. http://library7.open.ac.uk/abstracts/page.php?thesisid=52.
Pełny tekst źródłaSmith, 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.
Pełny tekst źródłaSymington, 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.
Pełny tekst źródłaFinke, 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.
Pełny tekst źródłaDe, Jong Sandra. "Accretion processes of radio galaxies at high energies". Phd thesis, Observatoire de Paris, 2013. http://tel.archives-ouvertes.fr/tel-00914365.
Pełny tekst źródłaAimar, 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.
Pełny tekst źródłaThe Milky Way, like presumably all structured galaxies, harbors a supermassive black hole at its core, approximately 4.3 million times the mass of the Sun, named Sagittarius A* (Sgr A*). Its size, determined by its mass, and its proximity of about 8.3 kpc make it the black hole with the largest angular size in the sky (~50 μas), making it the ideal target for studying this type of object. Black holes are the most compact objects in the Universe, with an extreme gravitational field near their event horizon. Describing these objects and their immediate environment requires taking into account General Relativity, introduced in 1915 by Albert Einstein .For over 20 years, Sgr A* and its environment have been the subject of numerous observation campaigns at various wavelengths (radio, IR, X-rays). Tracking the orbits of S-stars within one arcsecond around Sgr A* has provided evidence for certain effects predicted by General Relativity, such as Schwarzschild precession. X-ray and NIR observations have shown that Sgr A* exhibits significant variability in the emitted flux from the accretion flow. The advent of adaptive optics and optical interferometry, particularly with the four large telescopes of the VLTI and the GRAVITY instrument, have revealed an orbital motion of the origin of three flares observed in 2018.Numerous models have been proposed to explain the flares of Sgr A*, but the observation of orbital motion has strongly constrained these models. Among them, the analytical hot spot model is widely used with varying degrees of complexity and assumptions. In parallel with the development of analytical models, numerous simulations of accretion around black holes have been studied, with a particular focus on the phenomenon of magnetic reconnection, which appears as a plausible scenario to explain the origin of the flares of Sgr A*.In this thesis, we study different models for the flares of Sgr A* using the ray-tracing code Gyoto, ranging from an analytical hot spot model with intrinsic variability to a semi-analytical model based on magnetic reconnection. The first model is very useful for understanding the effects of Relativity (Special and General) on observables (astrometry and light curves), as well as the influence of intrinsic variability on them. The second model is motivated by a specific physical phenomenon, magnetic reconnection, and is constructed based on the results of numerical simulations. In this model, the azimuthal velocity is free to be super-Keplerian, due to the dragging of the reconnection site by the magnetic field lines. This property constitutes an observational constraint of the 2018 flares observed by GRAVITY that previous models failed to explain. Additionally, we also study the impact of modeling the quiescent state combined with the flares on the observables. Its contribution in astrometry calculations results in a shift between the position of the black hole and the center of the apparent orbit, which is another conclusion from the observations of the 2018 flares.In addition to astrometry and light curves, GRAVITY has measured the polarization of the 2018 flares. The Gyoto ray-tracing code is now capable of calculating the polarization of images. The new version of the code has been validated by comparing the results with another ray-tracing code, ipole.The model based on magnetic reconnection shows very promising results and can be further improved to account for polarization, as well as the multi-wavelength properties of the flares of Sgr A*
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.
Pełny tekst źródłaTomei, 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.
Pełny tekst źródłaKsiążki na temat "Accretion phenomena"
Beskin, Vassily, Gilles Henri, François Menard, Guy Pelletier i Jean Dalibard, red. Accretion discs, jets and high energy phenomena in astrophysics. Berlin, Heidelberg: Springer Berlin Heidelberg, 2003. http://dx.doi.org/10.1007/b80353.
Pełny tekst źródłaIAU 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. San Francisco, Calif: Astronomical Society of the Pacific, 1997.
Znajdź pełny tekst źródłaS, Beskin V., North Atlantic Treaty Organization. Scientific Affairs Division. i Nato Advanced Study Institute (2002 : Les Houches, Haute-Savoie, France)., red. 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. Les Ulis: EDP Sciences, 2003.
Znajdź pełny tekst źródła(Editor), Vassily Beskin, Gilles Henri (Editor), Francois Menard (Editor), Guy Pelletier (Editor) i Jean Dalibard (Editor), red. Accretion Disks, Jets and High-Energy Phenomena in Astrophysics (Les Houches - Ecole d'Ete de Physique Theorique). Springer, 2004.
Znajdź pełny tekst źródłaPelletier, Guy, Jean Dalibard, Gilles Henri, Vassily Beskin i Francois Menard. Accretion Disks, Jets and High-Energy Phenomena in Astrophysics: Les Houches Session LXXVIII, July 29 - August 23, 2002. Springer, 2010.
Znajdź pełny tekst źródła(Editor), Heon-Young Chang, Chang-Hwan Lee (Editor), Mannque Rho (Editor) i Insu Yi (Editor), red. 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.
Znajdź pełny tekst źródłaWickramasinghe, 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.
Znajdź pełny tekst źródłaTombesi, 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.
Znajdź pełny tekst źródłaCzęści książek na temat "Accretion phenomena"
Pringle, J. E. "Accretion Disc Phenomena". W Reviews in Modern Astronomy, 97–104. Berlin, Heidelberg: Springer Berlin Heidelberg, 1992. http://dx.doi.org/10.1007/978-3-642-77543-7_7.
Pełny tekst źródłaMineshige, S. "Accretion Disk Instabilities". W Nonlinear Phenomena in Stellar Variability, 83–103. Dordrecht: Springer Netherlands, 1993. http://dx.doi.org/10.1007/978-94-011-1062-4_8.
Pełny tekst źródłaKenyon, Scott J. "Accretion Disks and Eruptive Phenomena". W The Origin of Stars and Planetary Systems, 613–42. Dordrecht: Springer Netherlands, 1999. http://dx.doi.org/10.1007/978-94-011-4509-1_18.
Pełny tekst źródłaRebetzky, A., H. Herold, U. Kraus, H. P. Nollert i H. Ruder. "Accretion Phenomena at Neutron Stars". W Reviews in Modern Astronomy, 74–85. Berlin, Heidelberg: Springer Berlin Heidelberg, 1990. http://dx.doi.org/10.1007/978-3-642-76238-3_7.
Pełny tekst źródłaSchulz, Norbert S. "Accretion Phenomena and Magnetic Activity in YSOs". W The Formation and Early Evolution of Stars, 183–216. Berlin, Heidelberg: Springer Berlin Heidelberg, 2012. http://dx.doi.org/10.1007/978-3-642-23926-7_8.
Pełny tekst źródłaOkuda, T., i S. Mineshige. "Pulsational Instability of Accretion Disks Around Compact Objects". W Nonlinear Phenomena in Stellar Variability, 361–64. Dordrecht: Springer Netherlands, 1993. http://dx.doi.org/10.1007/978-94-011-1062-4_59.
Pełny tekst źródłaHeyvaerts, Jean. "Course 1: Accretion and Ejection-Related MHD". W Accretion discs, jets and high energy phenomena in astrophysics, 3–82. Berlin, Heidelberg: Springer Berlin Heidelberg, 2004. http://dx.doi.org/10.1007/978-3-540-39932-2_1.
Pełny tekst źródłaCzerny, Bozena. "Course 9: Accretion around Active Galactic Nuclei". W Accretion discs, jets and high energy phenomena in astrophysics, 461–90. Berlin, Heidelberg: Springer Berlin Heidelberg, 2004. http://dx.doi.org/10.1007/978-3-540-39932-2_9.
Pełny tekst źródłaHonma, F., R. Matsumoto i S. Kato. "Numerical Simulations of Pulsationally Unstable Accretion Disks Around Supermassive Black Holes". W Nonlinear Phenomena in Stellar Variability, 365–67. Dordrecht: Springer Netherlands, 1993. http://dx.doi.org/10.1007/978-94-011-1062-4_60.
Pełny tekst źródłaKudoh, T., i K. Shibata. "Magnetically Driven Jets From Accretion Disks: Nonsteady And Steady Solutions". W Magnetodynamic Phenomena in the Solar Atmosphere, 511–12. Dordrecht: Springer Netherlands, 1996. http://dx.doi.org/10.1007/978-94-009-0315-9_119.
Pełny tekst źródłaStreszczenia konferencji na temat "Accretion phenomena"
Vanbeveren, Dany. "Binaries, cluster dynamics and population studies of stars and stellar phenomena". W INTERACTING BINARIES: Accretion, Evolution, and Outcomes. AIP, 2005. http://dx.doi.org/10.1063/1.2130266.
Pełny tekst źródłaMeintjes, Pieter. "Magnetically driven transient phenomena in accretion driven systems: New breakthroughs with meerKAT and CTA?" W Accretion Processes in Cosmic Sources. Trieste, Italy: Sissa Medialab, 2018. http://dx.doi.org/10.22323/1.288.0039.
Pełny tekst źródłaHayashi, Ryosuke, i Makoto Yamamoto. "Numerical Simulation on Ice Accretion Phenomena in Rotor-Stator Interaction Field". W ASME Turbo Expo 2013: Turbine Technical Conference and Exposition. American Society of Mechanical Engineers, 2013. http://dx.doi.org/10.1115/gt2013-95448.
Pełny tekst źródłaChattopadhyay, Indranil, Mukesh Vyas i Kuldeep Singh. "Relativistic Jets From Black Hole Accretion Disc". W High Energy Phenomena in Relativistic Outflows VII. Trieste, Italy: Sissa Medialab, 2020. http://dx.doi.org/10.22323/1.354.0007.
Pełny tekst źródłaMeintjes, Pieter, i No Co-authors. "Magnetic reconnection and transient phenomena in accretion driven systems". W 4th Annual Conference on High Energy Astrophysics in Southern Africa. Trieste, Italy: Sissa Medialab, 2017. http://dx.doi.org/10.22323/1.275.0032.
Pełny tekst źródłaBoula, Stella, Demosthenes Kazanas, i Apostolos Mastichiadis. "Mhd Accretion Disk Winds And The Blazar Sequence". W High Energy Phenomena in Relativistic Outflows VII. Trieste, Italy: Sissa Medialab, 2020. http://dx.doi.org/10.22323/1.354.0009.
Pełny tekst źródłaTezok, F., M. Brahimi i I. Paraschivoiu. "Investigation of the physical processes underlying the ice accretion phenomena". W 36th AIAA Aerospace Sciences Meeting and Exhibit. Reston, Virigina: American Institute of Aeronautics and Astronautics, 1998. http://dx.doi.org/10.2514/6.1998-484.
Pełny tekst źródłaFuruta, Koharu, i Makoto Yamamoto. "Numerical Simulation on Ice Growth in High-Temperature Environment". W ASME Turbo Expo 2014: Turbine Technical Conference and Exposition. American Society of Mechanical Engineers, 2014. http://dx.doi.org/10.1115/gt2014-25847.
Pełny tekst źródłaFochi Wang, Yuzhen Lv, Qing Zhang, Zhou You i Chengrong Li. "Ice accretion on different aluminum cable steel reinforced". W 2010 IEEE Conference on Electrical Insulation and Dielectric Phenomena (CEIDP 2010). IEEE, 2010. http://dx.doi.org/10.1109/ceidp.2010.5723984.
Pełny tekst źródłaPark, Myeong-Gu. "Interaction of radiation with matter in accretion flow". W The first KIAS astrophysics workshop: Explosive phenomena in astrophysical compact objects. AIP, 2001. http://dx.doi.org/10.1063/1.1368268.
Pełny tekst źródłaRaporty organizacyjne na temat "Accretion phenomena"
Mayas, Magda. Creating with timbre. Norges Musikkhøgskole, sierpień 2018. http://dx.doi.org/10.22501/nmh-ar.686088.
Pełny tekst źródła