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Artykuły w czasopismach na temat "Black hole X-ray binaries"
Tanaka, Y. "Observation of Black Holes in X-ray Binaries". Symposium - International Astronomical Union 195 (2000): 37–47. http://dx.doi.org/10.1017/s007418090016276x.
Pełny tekst źródłaZiółkowski, Janusz, i Krzysztof Belczyński. "On the apparent lack of Be X-ray binaries with black holes in the galaxy and in the Magellanic Clouds". Proceedings of the International Astronomical Union 6, S275 (wrzesień 2010): 329–30. http://dx.doi.org/10.1017/s1743921310016340.
Pełny tekst źródłavan den Heuvel, Edward P. J. "High-Mass X-ray Binaries: progenitors of double compact objects". Proceedings of the International Astronomical Union 14, S346 (sierpień 2018): 1–13. http://dx.doi.org/10.1017/s1743921319001315.
Pełny tekst źródłaOrosz, Jerome A. "Inventory of black hole binaries". Symposium - International Astronomical Union 212 (2003): 365–71. http://dx.doi.org/10.1017/s0074180900212448.
Pełny tekst źródłaChen, Wen-Cong, i Xiang-Dong Li. "Evolution of black-hole intermediate-mass X-ray binaries". Proceedings of the International Astronomical Union 2, S238 (sierpień 2006): 339–40. http://dx.doi.org/10.1017/s1743921307005340.
Pełny tekst źródłaIvanova, Natalia. "Evolution of binaries with compact objects in globular clusters". Proceedings of the International Astronomical Union 10, S312 (sierpień 2014): 203–12. http://dx.doi.org/10.1017/s1743921315007826.
Pełny tekst źródłaRomani, Roger W. "The Formation and Evolution of Black-Hole Binaries". Symposium - International Astronomical Union 165 (1996): 93–103. http://dx.doi.org/10.1017/s0074180900055595.
Pełny tekst źródłaMakishima, Kazuo. "Observational evidence for intermediate-mass black holes: ultra-luminous X-ray sources". Proceedings of the International Astronomical Union 2, S238 (sierpień 2006): 209–18. http://dx.doi.org/10.1017/s1743921307004991.
Pełny tekst źródłaDotani, Tadayasu. "X-ray Observations of Black-Hole Binaries". Journal of the Korean Physical Society 54, nr 6(1) (15.06.2009): 2552–65. http://dx.doi.org/10.3938/jkps.54.2552.
Pełny tekst źródłaRemillard, Ronald A., i Jeffrey E. McClintock. "X-Ray Properties of Black-Hole Binaries". Annual Review of Astronomy and Astrophysics 44, nr 1 (wrzesień 2006): 49–92. http://dx.doi.org/10.1146/annurev.astro.44.051905.092532.
Pełny tekst źródłaRozprawy doktorskie na temat "Black hole X-ray binaries"
Klein-Wolt, Marc. "Black hole X-ray binaries". [S.l. : Amsterdam : s.n.] ; Universiteit van Amsterdam [Host], 2004. http://dare.uva.nl/document/91386.
Pełny tekst źródłaEGRON, ELISE MARIE JEANNE. "Spectral Comparisons of Neutron Star Low-Mass X-Ray Binaries with Black Hole X-Ray Binaries". Doctoral thesis, Università degli Studi di Cagliari, 2013. http://hdl.handle.net/11584/266223.
Pełny tekst źródłaDusoye, Avishek. "Accretion and outflow in black-hole x-ray binaries". Master's thesis, University of Cape Town, 2015. http://hdl.handle.net/11427/15518.
Pełny tekst źródłaKnevitt, Gillian Frances Grace. "Black hole X-ray binaries : radiation and high-redshift feedback". Thesis, University of Leicester, 2014. http://hdl.handle.net/2381/29158.
Pełny tekst źródłaShidatsu, Megumi. "Observational Studies of Accretion Disks in Black Hole X-ray Binaries". 京都大学 (Kyoto University), 2015. http://hdl.handle.net/2433/199106.
Pełny tekst źródłaMiller, Jon Matthew 1975. "X-ray spectroscopic and timing studies of galactic black hole binaries". Thesis, Massachusetts Institute of Technology, 2002. http://hdl.handle.net/1721.1/29935.
Pełny tekst źródłaIncludes bibliographical references (p. 183).
In rare cases, optical observations of Galactic binary star systems which are bright in the X-ray portion of the electromagnetic spectrum dynamically constrain the mass of one component to be well above theoretical limits for a neutron star. These systems - and systems with similar X-ray properties - are classified as black hole binaries. In this thesis, I report on observations of black hole binaries made with satellite observatories in the X-ray band. The region closest to the black hole is revealed in X-rays due to the viscous heating of matter that is accreted from the companion star. X-ray observations of these systems may therefore reveal General Relativistic effects. A fundamental and testable prediction of General Relativity is that matter may orbit more closely around black holes with significant angular momentum. I have investigated the possibility of black hole "spin" and the geometry of accretion flows in these systems using X-ray continuum spectroscopy, fast variability studies, and the shape of iron fluorescent emission lines in this band. I present evidence for black hole spin in XTE J1550-564, XTE J1650-500, and XTE J1748-248. Spin is not required by high-resolution spectral analysis of the archetypical Galactic black hole - Cygnus X-1 but a thermal accretion disk plus hot corona geometry is confirmed. Studies of XTE J1118+480 and GRS 1758-258 at low X-ray luminosity reveal that models for radiatively-inefficient accretion do not satisfactorily describe the geometry in these systems.
y Jon Matthew Miller.
Ph.D.
Brocksopp, Catherine. "Multiwavelength variability of black hole x-ray binaries in the low/hard state". Thesis, [n.p.], 2000. http://oro.open.ac.uk/19112/.
Pełny tekst źródłaMARINO, ALESSIO. "Imperfect accretion: ejecting matter in X-ray binaries". Doctoral thesis, Università degli Studi di Palermo, 2021. http://hdl.handle.net/10447/479017.
Pełny tekst źródłaDijk, Robertus Cornelis Adrianus van. "Gamma-ray observations of x-ray binaries with COMPTEL a study of black-hole candidates and 2CG 135+01 /". Amsterdam : Utrecht : Amsterdam : Sterrenkundig Instituut "Anton Pannekoek", Universiteit van Amsterdam ; Stichting Ruimteonderzoek Nederland ; Universiteit van Amsterdam [Host], 1996. http://dare.uva.nl/document/91713.
Pełny tekst źródłaBurke, Mark J. "Extragalactic X-ray binaries : black holes and neutron stars in Centaurus A". Thesis, University of Birmingham, 2013. http://etheses.bham.ac.uk//id/eprint/4496/.
Pełny tekst źródłaKsiążki na temat "Black hole X-ray binaries"
A, Nowak Michael, i United States. National Aeronautics and Space Administration., red. X-ray variability coherence: How to compute it, what it means, and how it constrains models of GX 339-4 and Cygnus X-1. [Washington, DC: National Aeronautics and Space Administration, 1997.
Znajdź pełny tekst źródłaA, Nowak Michael, i United States. National Aeronautics and Space Administration., red. X-ray variability coherence: How to compute it, what it means, and how it constrains models of GX 339-4 and Cygnus X-1. [Washington, DC: National Aeronautics and Space Administration, 1997.
Znajdź pełny tekst źródłaA, Nowak Michael, i United States. National Aeronautics and Space Administration., red. X-ray variability coherence: How to compute it, what it means, and how it constrains models of GX 339-4 and Cygnus X-1. [Washington, DC: National Aeronautics and Space Administration, 1997.
Znajdź pełny tekst źródłaUnited States. National Aeronautics and Space Administration., red. A search for periodicity in the X-ray spectrum of black hole candidate A0620-00. [Washington, DC: National Aeronautics and Space Administration, 1991.
Znajdź pełny tekst źródłaInvestigating the Physics of Hard X-ray Outbursts from the Galactic Center Supermassive Black Hole Sagittarius A*. [New York, N.Y.?]: [publisher not identified], 2016.
Znajdź pełny tekst źródłaUnited States. National Aeronautics and Space Administration., red. Is there a supermassive black hole in the nucleus of M31?: NASA grant NAG5-2673 : final report for the period 15 August 1994 through 14 August 1997. Cambridge, Mass: Smithsonian Institution, Astrophysical Observatory, 1997.
Znajdź pełny tekst źródłaNational Aeronautics and Space Administration (NASA) Staff. Relativistic Astrophysics in Black Hole and Low-Mass Neutron Star X-Ray Binaries. Independently Published, 2018.
Znajdź pełny tekst źródłaHo, Luis C., Thomas J. Maccarone i Robert P. Fender. From X-ray Binaries to Quasars: Black Holes on All Mass Scales. Springer, 2008.
Znajdź pełny tekst źródła(Editor), Thomas J. Maccarone, Robert P. Fender (Editor) i Luis C. Ho (Editor), red. From X-ray Binaries to Quasars: Black Holes on All Mass Scales. Springer, 2006.
Znajdź pełny tekst źródłaCzęści książek na temat "Black hole X-ray binaries"
Tanaka, Y. "Black-Hole Binaries". W The Universe in X-Rays, 237–59. Berlin, Heidelberg: Springer Berlin Heidelberg, 2008. http://dx.doi.org/10.1007/978-3-540-34412-4_16.
Pełny tekst źródłaTauris, T. M., i G. J. Savonije. "Spin-Orbit Couplings in X-Ray Binaries". W The Neutron Star—Black Hole Connection, 337–42. Dordrecht: Springer Netherlands, 2001. http://dx.doi.org/10.1007/978-94-010-0548-7_25.
Pełny tekst źródłaGilfanov, M. "X-Ray Emission from Black-Hole Binaries". W The Jet Paradigm, 17–51. Berlin, Heidelberg: Springer Berlin Heidelberg, 2009. http://dx.doi.org/10.1007/978-3-540-76937-8_2.
Pełny tekst źródłaBildsten, L., i R. E. Rutledge. "Transient Low-Mass X-Ray Binaries in Quiescence". W The Neutron Star—Black Hole Connection, 245–60. Dordrecht: Springer Netherlands, 2001. http://dx.doi.org/10.1007/978-94-010-0548-7_14.
Pełny tekst źródłaGilfanov, M., E. Churazov i R. Sunyaev. "X-ray Spectral Variability of Black Hole Binaries". W Observational Evidence for Black Holes in the Universe, 319–40. Dordrecht: Springer Netherlands, 1999. http://dx.doi.org/10.1007/978-94-011-4750-7_23.
Pełny tekst źródłaSpruit, H. C. "Gamma-Ray Bursts from Neutron Stars Spun up in X-Ray Binaries". W The Neutron Star—Black Hole Connection, 467–74. Dordrecht: Springer Netherlands, 2001. http://dx.doi.org/10.1007/978-94-010-0548-7_33.
Pełny tekst źródłavan Paradijs, J. "Black holes in X-ray binaries". W Accretion Disks — New Aspects, 21–35. Berlin, Heidelberg: Springer Berlin Heidelberg, 1997. http://dx.doi.org/10.1007/bfb0105818.
Pełny tekst źródłaMcClintock, Jeffrey E. "Black Holes in Binary Systems". W X-Ray Binaries and Recycled Pulsars, 27–36. Dordrecht: Springer Netherlands, 1992. http://dx.doi.org/10.1007/978-94-011-2704-2_3.
Pełny tekst źródłaVolwerk, Martin, Roeland Oss i Jan Kuijpers. "Magnetic Flares Near Black Holes". W X-Ray Binaries and Recycled Pulsars, 537. Dordrecht: Springer Netherlands, 1992. http://dx.doi.org/10.1007/978-94-011-2704-2_47.
Pełny tekst źródłaMÉndez, M. "Timing the Kilohertz Quasi-Periodic Oscillations in Low-Mass X-Ray Binaries". W The Neutron Star—Black Hole Connection, 313–18. Dordrecht: Springer Netherlands, 2001. http://dx.doi.org/10.1007/978-94-010-0548-7_21.
Pełny tekst źródłaStreszczenia konferencji na temat "Black hole X-ray binaries"
Gallo, Elena. "Black hole X-ray binary jets". W INTERACTING BINARIES: Accretion, Evolution, and Outcomes. AIP, 2005. http://dx.doi.org/10.1063/1.2130232.
Pełny tekst źródłaNowak, Michael A. "Modeling black hole x-ray power spectra". W The evolution of X-ray binaries. AIP, 1994. http://dx.doi.org/10.1063/1.45937.
Pełny tekst źródłaMukai, Koji. "Application of magnetic braking theories to black hole binaries". W The evolution of X-ray binaries. AIP, 1994. http://dx.doi.org/10.1063/1.45992.
Pełny tekst źródłaShahbaz, T., T. Naylor i P. A. Charles. "The mass of the black hole in A0620-00". W The evolution of X-ray binaries. AIP, 1994. http://dx.doi.org/10.1063/1.46029.
Pełny tekst źródłaEbisawa, Ken. "X-ray energy spectra from accretion disks in black hole candidates". W The evolution of X-ray binaries. AIP, 1994. http://dx.doi.org/10.1063/1.46000.
Pełny tekst źródłaCesares, J., i P. A. Charles. "The mass of the black hole in GS2023+338/V404 Cygni". W The evolution of X-ray binaries. AIP, 1994. http://dx.doi.org/10.1063/1.46026.
Pełny tekst źródłaMENOU, KRISTEN. "BLACK HOLE ACCRETION IN TRANSIENT X-RAY BINARIES". W Proceedings of the 2nd KIAS Astrophysics Workshop. WORLD SCIENTIFIC, 2002. http://dx.doi.org/10.1142/9789812777959_0008.
Pełny tekst źródłaBelloni, Tomaso M., Sara Motta, Jéro^me Rodriguez i Phillippe Ferrando. "Black-hole Binaries: Life Begins at 40 keV". W SIMBOL-X: FOCUSING ON THE HARD X-RAY UNIVERSE: Proceedings of the 2nd International Simbol-X Symposium. AIP, 2009. http://dx.doi.org/10.1063/1.3149408.
Pełny tekst źródłaGrebenev, Sergei A., Rashid A. Sunyaev i Mikhail N. Pavlinsky. "Observational constraints on the models of disk accretion onto a black hole". W The evolution of X-ray binaries. AIP, 1994. http://dx.doi.org/10.1063/1.45949.
Pełny tekst źródłaLuo, Chuan, Cesar Meirelles i Edison Liang. "X-ray transitions of black hole binaries and variable α-parameter disks". W The evolution of X-ray binaries. AIP, 1994. http://dx.doi.org/10.1063/1.45991.
Pełny tekst źródłaRaporty organizacyjne na temat "Black hole X-ray binaries"
Tournear, Derek M. X-ray Bursts in Neutron Star and Black Hole Binaries from USA Data: Detections and Upper Limits. Office of Scientific and Technical Information (OSTI), luty 2003. http://dx.doi.org/10.2172/813180.
Pełny tekst źródłaVollrath, Z. Black Hole Accretion and X-Ray Variability in AGN. Office of Scientific and Technical Information (OSTI), wrzesień 2004. http://dx.doi.org/10.2172/833107.
Pełny tekst źródłaShabad, Gayane. High-Frequency X-ray Variability Detection in A Black Hole Transient with USA. Office of Scientific and Technical Information (OSTI), październik 2000. http://dx.doi.org/10.2172/784707.
Pełny tekst źródłaShabad, G. High-Frequency X-ray Variability Detection in A Black Hole Transient with USA. Office of Scientific and Technical Information (OSTI), czerwiec 2018. http://dx.doi.org/10.2172/1454236.
Pełny tekst źródłaReilly, Kaice T. X-Ray Timing and Spectral Observations of Galactic Black Hole Candidate XTE J1550--564 During Outburst. Office of Scientific and Technical Information (OSTI), grudzień 2002. http://dx.doi.org/10.2172/808722.
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