A Relativistic Fe Kα Emission Line in the Intermediate-Luminosity BeppoSAX Spectrum of the Galactic Microquasar V4641 Sgr
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U. Maryland | A. Fabian | J. Miller | R. Wijnands | J. Zand | C. Reynolds | W. Lewin | M. Nowak | Sron | Univ. of Cambridge IoA | J. I. '. in ’t Zand | W.H.G. Lewin Mit Csr | Utrecht Univ. | J. Miller | J. I. ’. in ’t Zand
[1] Merate,et al. Evidence for a relativistic iron line in GRS 1915+105 , 2002, astro-ph/0203185.
[2] M. J. Freyberg,et al. Evidence of Spin and Energy Extraction in a Galactic Black Hole Candidate: The XMM-Newton/EPIC-pn Spectrum of XTE J1650–500 , 2002, astro-ph/0202375.
[3] M. Nowak,et al. Coronal-temporal correlations in GX 339-4: hysteresis, possible reflection changes and implications for advection-dominated accretion flows , 2002, astro-ph/0201383.
[4] A. Fabian,et al. Fe Kα emission from photoionized slabs: the impact of the iron abundance , 2001, astro-ph/0112179.
[5] Moscow,et al. V4641Sgr - A super-Eddington source enshrouded by an extended envelope , 2001, astro-ph/0109269.
[6] J. Gelbord,et al. Variable Iron Kα Lines in Seyfert 1 Galaxies , 2000, astro-ph/0008522.
[7] Charles D. Bailyn,et al. A Black Hole in the Superluminal Source SAX J1819.3–2525 (V4641 Sgr) , 2000, astro-ph/0103045.
[8] Simon T. Garrington,et al. Light Curves and Radio Structure of the 1999 September Transient Event in V4641 Sagittarii (=XTE J1819–254=SAX J1819.3–2525) , 2000 .
[9] Andrew C. Fabian,et al. Broad Iron Lines in Active Galactic Nuclei , 2000 .
[10] R. Wijnands,et al. Correlated X-Ray Spectral and Timing Behavior of the Black Hole Candidate XTE J1550–564: A New Interpretation of Black Hole States , 2000, astro-ph/0001163.
[11] Lev Titarchuk,et al. Mass Determination of Black Holes in LMC X-1 and Nova Muscae 1991 from Their High-Energy Spectra , 1999, astro-ph/9906275.
[12] A. Fabian,et al. Variation of the broad X-ray iron line in MCG-6-30-15 during a flare , 1999, astro-ph/9904078.
[13] Astronomy,et al. Progressive covering of the accretion disc corona during dipping in the LMXB XB 1916–053 , 1998, astro-ph/9810185.
[14] R. Narayan,et al. Advection-Dominated Accretion and the Spectral States of Black Hole X-Ray Binaries: Application to Nova Muscae 1991 , 1997, astro-ph/9705237.
[15] J. Poutanen,et al. The Two-Phase Pair Corona Model for Active Galactic Nuclei and X-ray Binaries: How to Obtain Exact Solutions , 1996, astro-ph/9605073.
[16] Lev Titarchuk,et al. GENERALIZED COMPTONIZATION MODELS AND APPLICATION TO THE RECENT HIGH-ENERGY OBSERVATIONS , 1994 .
[17] Chris Biemesderfer,et al. Astronomical Data Analysis Software and Systems X , 2001 .
[18] A. Laor. Line Profiles from a Disk around a Rotating Black Hole , 1991 .
[19] J. Dickey,et al. H I in the Galaxy , 1990 .
[20] Nicholas E. White,et al. X-ray fluorescence from the inner disc in Cygnus X-1 , 1989 .