X-ray novae

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[20]  N. Nakamura.  Tenma Observation of X-Ray Bursts from X1608-52 , 1989 .

[21]  J. B. Oke.  Further spectrophotometry of the transient X-ray source A0620-00 , 1977 .

[22]  Kazuhisa Mitsuda,et al.  Luminosity-related changes of the energy spectrum of X1608-522 , 1989 .

[23]  M. Turner,et al.  The X-ray spectrum of A0620—00 , 1975, Nature.

[24]  J. Casares,et al.  Optical studies of V404 Cyg, the X-Ray transient GS 2023 + 338 – III. The secondary star and accretion disc , 1993 .

[25]  F. A. Cordova,et al.  Transient radio emission from the X-ray nova ASM 2000+25 , 1988 .

[26]  J. Wheeler,et al.  Accretion disks in compact stellar systems , 1993 .

[27]  P. Callanan,et al.  The soft X-ray transient GS2000+25. II, An ellipsoidal modulation in quiescence , 1991 .

[28]  C. T. Bolton,et al.  The optical spectrum of HDE 226868 = Cygnus X-1. I - Radial velocities and orbital elements , 1982 .

[29]  S. Kitamoto,et al.  The Unstable Long-Term Periodicity of Aquila X-1 , 1993 .

[30]  John K. Cannizzo,et al.  The Limit Cycle Instability in Dwarf Nova Accretion Disks , 1993 .

[31]  W. Liller.  Searches for the optical counterparts of the X-ray burst sources MXB 1728-34 and MXB 1730-33 , 1977 .

[32]  M. Turner,et al.  Discovery of powerful transient X-ray source A0620—00 with Ariel V Sky Survey Experiment , 1975, Nature.

[33]  H. Marshall,et al.  Dual character of the rapid burster and a classification of X-ray bursts , 1978, Nature.

[34]  C. Bailyn,et al.  Evidence for a black hole in the X-ray binary Nova Muscae 1991 , 1992 .

[35]  J. Grindlay,et al.  Discovery of the optical counterpart of the transient X-ray burster Centaurus X-4 , 1980 .

[36]  L. Stella,et al.  The X-ray spectral properties of accretion discs in X-ray binaries , 1988 .

[37]  A. Cowley.  Evidence for Black Holes in Stellar Binary Systems , 1992 .

[38]  A. Finoguenov,et al.  Hard X-ray variability of X-ray Nova Persei 1992: GRANAT/SIGMA results , 1995 .

[39]  A. R. King,et al.  The evolutionary status of the black hole candidate V404 Cygni , 1993 .

[40]  D. J. Helfand,et al.  A soft X-ray study of the Large Magellanic Cloud , 1981 .

[41]  M. Tavani,et al.  On the nature and evolution of the windy binary pulsar PSR 1744 - 24A , 1991 .

[42]  M. Livio,et al.  The secondary maxima in black hole X-ray nova light curves , 1993 .

[43]  J. Wheeler,et al.  Disk-instability model for soft-X-ray transients containing black holes , 1989 .

[44]  E. M. Jones,et al.  Radio emission from young supernova remnants - Effects of an inhomogeneous circumstellar medium , 1989 .

[45]  M. Colpi,et al.  Do quiescent soft X-ray transients contain millisecond radio pulsars? , 1994 .

[46]  G. Ricker,et al.  Periodic variability of the X-ray nova A 0620-00 in quiescence , 1983 .

[47]  R. Sunyaev,et al.  Why the number of galactic X-ray stars is so small , 1975 .

[48]  S. Howell,et al.  ROSAT observations of the black hole candidate V404 Cygni in quiescence , 1994 .

[49]  Y. Osaki.  An Accretion Model for the Outbursts of U Geminorum Stars , 1974 .

[50]  I. Morison,et al.  Observations of A0620—00 at 962 and 151 MHz , 1975, Nature.

[51]  D. Crampton,et al.  Optical and UV spectroscopy of the black hole binary candidate LMC X-1 , 1987 .

[52]  J. McClintock,et al.  The X-Ray Nova Centaurus X-4: Comparisons with A0620-00 , 1990 .

[53]  J. Thorstensen,et al.  The optical counterpart of Aquila X-1 /3U 1908+00/ , 1978 .

[54]  S. Howell,et al.  Optical identification of the X-ray source GS 2023+338 as V404 Cygni , 1991 .

[55]  A. King,et al.  A model for soft X-ray transients , 1986 .

[56]  J. Casares,et al.  A 6.5-day periodicity in the recurrent nova V404 Cygni implying the presence of a black hole , 1992, Nature.

[57]  D. Crampton,et al.  An Orbital Model for the X-Ray Transient CEN X-4 , 1988 .

[58]  R. Fujimoto,et al.  Low State Properties of the Low-Mass X-Ray Binary X1608-522 Observed with Ginga , 1993 .

[59]  Rashid Sunyaev,et al.  Black holes in binary systems. Observational appearance , 1973 .

[60]  D. Crampton,et al.  Discovery of a massive unseen star in LMC X-3 , 1983 .

[61]  D. Roussel-Dupre,et al.  Recurrence times and periodicities in 4U 1608-52 as observed by Vela 5B , 1994 .

[62]  G. Clark,et al.  The transient X-ray source A0620-00 - Intensity variations and evidence for an 8 day periodicity , 1976 .

[63]  J. Wheeler,et al.  Thermal instability accretion disk model for the X-ray transient A0620-00 , 1989 .

[64]  M. C. Begam,et al.  The optical counterpart of the superluminal source GRO J1655 – 40 , 1995, Nature.

[65]  I. Mirabel,et al.  A superluminal source in the Galaxy , 1994, Nature.

[66]  R. M. Hjellming,et al.  Episodic ejection of relativistic jets by the X-ray transient GRO J1655 - 40 , 1995, Nature.

[67]  J. McClintock,et al.  The Black Hole Binary A0620-00 , 1986 .

[68]  Thomas Matheson,et al.  The Mass of the Probable Black Hole in the X-Ray Nova GRO J0422+32 , 1995 .

[69]  K. Mitsuda,et al.  ASCA Observations of Soft X-Ray Transients in Quiescence : X1608-52 and CEN X-4 , 1996 .

[70]  S. Hayakawa,et al.  Discovery of X-Ray Bursts from AQUILA X-1 , 1981 .

[71]  N. Khavenson,et al.  X-ray nova in Musca (GRS 1124 - 68) - Hard X-ray source with narrow annihilation line , 1992 .

[72]  A. Henden,et al.  Near-quiescent photometry of the X-ray transient J0422+32 , 1995 .

[73]  H. Bradt,et al.  Optical identification of A0620-00 , 1976 .

[74]  K. Koyama,et al.  Discovery of a large X-ray burst from an X-ray nova, Centaurus X-4 , 1980 .

[75]  S. Kitamoto,et al.  GS2023+338: a new class of X-ray transient source? , 1989, Nature.

[76]  A. King,et al.  Soft X-ray transients and the evolution of low mass X-ray binaries , 1987 .

[77]  S. Holt,et al.  The 1979 X-ray outburst of Centaurus X-4 , 1980 .

[78]  J. Cannizzo,et al.  Accretion Instability Models for Dwarf Novae and X-Ray Transients , 1982 .

[79]  G. J. Fishman,et al.  Correlations between X-ray outbursts and relativistic ejections in the X-ray transient GRO J1655 – 40 , 1995, Nature.

[80]  Michael R. Garcia,et al.  Observations of the X-ray Nova GRO J0422+32. 1: Outburst and the decay to quiescence , 1995 .

[81]  K. Horne,et al.  The dim inner accretion disk of the quiescent black hole A0620-00 , 1995 .

[82]  T. Marsh,et al.  Doppler tomography of the X-ray transient J0422+32 during the 1993 December mini-outburst , 1995 .

[83]  Thomas J. Balonek,et al.  Radio emission from the X-ray source A0620-00. , 1976 .

[84]  Shin Mineshige,et al.  Black Hole Accretion Disk Instabilities , 1993 .

[85]  Hans Ritter,et al.  The light curves of soft X‐ray transients , 1988 .

[86]  Ramesh Narayan,et al.  A New Model for Black Hole Soft X-Ray Transients in Quiescence , 1995, astro-ph/9508014.

[87]  E. L. Wright,et al.  Optical observations of the recurrent Nova associated with A0620-00 : 1917-1975. , 1976 .

[88]  S. Kitamoto,et al.  Spectral Evolution of the Bright X-Ray Nova GS 1124-68 (Nova MUSCAE 1991) Observed with GINGA , 1994 .

[89]  W. Priedhorsky,et al.  Long-term observations of x-ray sources: The aquila-serpens-scutum region , 1984 .

[90]  S. Kitamoto,et al.  Discovery and x-ray properties of GS 1124-683 (= Nova Muscae) , 1992 .

[91]  T. Courvoisier,et al.  Multi-Wavelength Continuum Emission of AGN , 1994 .

[92]  Walter H. G. Lewin,et al.  X-ray binaries. , 1976 .

[93]  William C. Priedhorsky,et al.  Long-term cycles in cosmic X-ray sources , 1987 .

[94]  K. Arnaud,et al.  Soft X-ray transients in quiescence: observations of Aql X-1 and Cen X-4 , 1987 .