A Black Hole in the Superluminal Source SAX J1819.3–2525 (V4641 Sgr)
暂无分享,去创建一个
Charles D. Bailyn | Ronald A. Remillard | Michael R. Garcia | Jerome A. Orosz | Erik Kuulkers | J. Orosz | C. Bailyn | R. Jain | E. Kuulkers | J. McClintock | P. Callanan | R. Remillard | Michiel van der Klis | Jeffrey E. McClintock | Raj K. Jain | Michael R. Garcia Paul J. Callanan | M. van der Klis | J. Mcclintock
[1] N. Lomb. Least-squares frequency analysis of unequally spaced data , 1976 .
[2] A. Stark,et al. The rotation curve of the Milky Way to 2 R(0) , 1989 .
[3] Tim Naylor,et al. The mass of the black hole in V404 Cygni , 1994 .
[4] Charles D. Bailyn,et al. THE MASS DISTRIBUTION OF STELLAR BLACK HOLES , 1998 .
[5] 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 .
[6] L. Natalucci,et al. Bursting sources in the Galactic Centre region , 1999 .
[7] A TiO study of the black hole binary GRO J0422+32 in a very low state , 2000, astro-ph/0004235.
[8] J. Orosz,et al. Orbital Parameters for the Soft X-Ray Transient 4U 1543–47: Evidence for a Black Hole , 1997, astro-ph/9712018.
[9] P. H. Hauschildt,et al. Numerical solution of the expanding stellar atmosphere problem , 1998 .
[10] R. M. Hjellming,et al. Episodic ejection of relativistic jets by the X-ray transient GRO J1655 - 40 , 1995, Nature.
[11] J. McClintock,et al. The Black Hole Binary A0620-00 , 1986 .
[12] R. Stellingwerf. Period determination using phase dispersion minimization , 1978 .
[13] J. Orosz,et al. Improved Parameters for the Black Hole Binary System X-Ray Nova MUSCAE 1991 , 1996 .
[14] J. Scargle. Studies in astronomical time series analysis. II - Statistical aspects of spectral analysis of unevenly spaced data , 1982 .
[15] Charles D. Bailyn,et al. Optical and Infrared Photometry of the Microquasar GRO J1655-40 in Quiescence , 2001 .
[16] Astronomy,et al. Multiepoch Very Long Baseline Array Observations of EGRET-detected Quasars and BL Lacertae Objects: Superluminal Motion of Gamma-Ray Bright Blazars , 2001, astro-ph/0101570.
[17] J. Tonry,et al. A survey of galaxy redshifts. I. Data reduction techniques. , 1979 .
[18] I. Mirabel,et al. Sources of Relativistic Jets in the Galaxy , 1999, astro-ph/9902062.
[19] P. Szkody,et al. Spectroscopy of Poorly Studied Cataclysmic Variables , 1995 .
[20] Eduardo L. Martin,et al. Evidence of a supernova origin for the black hole in the system GRO J1655 - 40 , 1999, Nature.
[21] J. Tomkin,et al. The chemical composition of algol systems – III. Beta Lyrae–nucleosynthesis revealed , 1986 .
[22] D. Fabricant,et al. The FAST Spectrograph for the Tillinghast Telescope , 1998 .
[23] Robert L. Kurucz,et al. A calibration of Geneva photometry for B to G stars in terms of Teff, log g and $[M/H]$ , 1997 .
[24] Lothar Noethe,et al. Active optics. Pt. 4. Set-up and performance of the optics of the ESO New Technology Telescope (NTT) in the observatory. , 1991 .
[25] E. L. Robinson,et al. On the mass of the compact object in the black hole binary A0620-00 , 1993 .
[26] J. Wheeler. Supernovae and Gamma-Ray Bursts , 2000 .
[27] J. Hartle,et al. Stationary configurations and the upper bound on the mass of nonrotating, causal neutron stars , 1976 .
[28] C. Simon Jeffery,et al. Newsletter on Analysis of Astronomical Spectra , 1996 .
[29] J. Orosz,et al. Optical Observations of GRO J1655–40 in Quiescence. I. A Precise Mass for the Black Hole Primary , 1996, astro-ph/9610211.
[30] Rudy WijnandsMichiel van der Klis. The Rapid X-Ray Variability of V4641 Sagittarii (SAX J1819.3-2525 = XTE J1819-254). , 2000 .
[31] E. L. Robinson,et al. Spectroscopy of $A0620-00$: the mass of the black hole and an image of its accretion disc , 1994 .
[32] D. F. Gray,et al. The Observation and Analysis of Stellar Photospheres , 2021 .