Transient Low-Mass X-Ray Binaries in Quiescence
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[1] R. Rutledge,et al. No Persistent Pulsations in Aquila X-1 As It Fades into Quiescence , 2000, astro-ph/0010555.
[2] L. Bildsten,et al. Coronal X-Ray Emission from the Stellar Companions to Transiently Accreting Black Holes , 1999, astro-ph/9912304.
[3] L. Bildsten,et al. A Method for Distinguishing between Transiently Accreting Neutron Stars and Black Holes, in Quiescence , 1999, astro-ph/9909319.
[4] Michael R. Garcia,et al. Two Neutron Star Soft X-Ray Transients in Quiescence: 4U 2129+47 and EXO 0748−676 , 1999, astro-ph/9904117.
[5] UK.,et al. An eclipse of the X-ray flux from the dwarf nova OY Carinae in quiescence , 1999, astro-ph/9903058.
[6] S. Drake,et al. X-Ray Spectroscopy of Rapidly Rotating, Late-Type Dwarf Stars , 1999 .
[7] Yasuo Tanaka,et al. ASCA Observations of Transient X-Ray Sources in Quiescence , 1998 .
[8] R. Narayan,et al. Thermal X-Ray Line Emission from Accreting Black Holes , 1998, astro-ph/9811412.
[9] Kristen Menou,et al. Black Hole and Neutron Star Transients in Quiescence , 1998, astro-ph/9810323.
[10] L. Bildsten,et al. The Thermal X-Ray Spectra of Centaurus X-4, Aquila X-1 , and 4U 1608-522 in Quiescence , 1998, astro-ph/9810288.
[11] D. Psaltis,et al. The Disk-Magnetosphere Interaction in the Accretion-powered Millisecond Pulsar SAX J1808.4–3658 , 1998, astro-ph/9809335.
[12] L. Bildsten,et al. Crustal Heating and Quiescent Emission from Transiently Accreting Neutron Stars , 1998, astro-ph/9807179.
[13] R. Wijnands,et al. A millisecond pulsar in an X-ray binary system , 1998, Nature.
[14] E. Morgan,et al. The two-hour orbit of a binary millisecond X-ray pulsar , 1998, Nature.
[15] M. Colpi,et al. Aquila X-1 from outburst to quiescence: the onset of the propeller effect and signs of a turned-on rotation-powered pulsar , 1998, astro-ph/9803303.
[16] Yu Wang,et al. Spectral State Transitions in Aquila X-1: Evidence for “Propeller” Effects , 1998 .
[17] R. Kelley,et al. Millisecond Oscillations in the Persistent and Bursting Flux of Aquila X-1 during an Outburst , 1997, astro-ph/9712300.
[18] M. Livio,et al. The Properties of X-Ray and Optical Light Curves of X-Ray Novae , 1997, astro-ph/9707138.
[19] B. Thomas,et al. Discovery of a New Soft X-Ray Excess in the Spectrum of EXO 0748–676 , 1997 .
[20] R. Narayan,et al. Advection-dominated Flows around Black Holes and the X-Ray Delay in the Outburst of GRO J1655–40 , 1997, astro-ph/9703095.
[21] Tim Naylor,et al. The X-Ray Eclipse of the Dwarf Nova HT Cassiopeiae: Results from ASCA and ROSAT HRI Observations , 1997 .
[22] Michael R. Garcia,et al. � 1997. The American Astronomical Society. All rights reserved. Printed in U.S.A. ADVECTION-DOMINATED ACCRETION AND BLACK HOLE EVENT HORIZONS , 1996 .
[23] J. Grindlay,et al. Luminosity Differences Between Black Holes and Neutron Stars , 1996 .
[24] R. Narayan,et al. Advection-dominated Accretion Model of the Black Hole V404 Cygni in Quiescence , 1996, astro-ph/9610014.
[25] L. Bildsten,et al. Thermonuclear Burning on the Accreting X-Ray Pulsar GRO J1744–28 , 1996, astro-ph/9609155.
[26] Yasuo Tanaka,et al. X-ray novae , 1996 .
[27] Luciano Burderi,et al. Black Hole Binaries and X-Ray Transients , 1996 .
[28] J. van Paradijs,et al. On the Accretion Instability in Soft X-Ray Transients , 1996 .
[29] K. Mitsuda,et al. ASCA Observations of Soft X-Ray Transients in Quiescence : X1608-52 and CEN X-4 , 1996 .
[30] J. Grindlay,et al. Spectroscopic Identification of Probable Cataclysmic Variables in the Globular Cluster NGC 6397 , 1995 .
[31] R. Romani,et al. Model atmospheres for low field neutron stars , 1995, astro-ph/9510094.
[32] K. Horne,et al. The dim inner accretion disk of the quiescent black hole A0620-00 , 1995 .
[33] A. Cool,et al. Discovery of candidate cataclysmic variables in the post-core-collapse globular cluster NGC 6397 , 1995 .
[34] T. Dotani,et al. Is the changing orbital period of EXO 0748-676 evidence for a triple system? , 1994 .
[35] A. Treves,et al. X-Ray Spectra from Neutron Stars Accreting at Low Rates , 1994, astro-ph/9407067.
[36] S. Howell,et al. ROSAT observations of the black hole candidate V404 Cygni in quiescence , 1994 .
[37] M. Colpi,et al. Do quiescent soft X-ray transients contain millisecond radio pulsars? , 1994 .
[38] S. Campana,et al. The neutron stars of Soft X–ray Transients , 1993, astro-ph/9805079.
[39] J. Wheeler,et al. Disk-instability model for soft-X-ray transients containing black holes , 1989 .
[40] J. Wheeler,et al. Thermal instability accretion disk model for the X-ray transient A0620-00 , 1989 .
[41] O. Vilhu,et al. Chromospheric-coronal activity at saturated levels , 1987 .
[42] R. Romani. Model atmospheres for cooling neutron stars , 1987 .
[43] R. Rosner,et al. Intermittent stellar wind accretion and the long-term activity of Population I binary systems containing an X-ray pulsar , 1986 .
[44] J. Patterson,et al. X-ray emission from cataclysmic variables with accretion disks. II. EUV/Soft x-ray radiation , 1985 .
[45] F. Verbunt. X-ray sources in globular clusters , 1984, astro-ph/0111439.
[46] Keith O. Mason,et al. X-ray observations of a large sample of cataclysmic variable stars using the Einstein Observatory , 1984 .
[47] J. Grindlay,et al. X-ray evidence for white dwarf binaries in globular clusters , 1983 .
[48] C. Alcock,et al. The surface chemistry of stars. I - Diffusion of heavy ions in white dwarf envelopes. II - Fractionated accretion of interstellar matter , 1980 .
[49] Barham W. Smith,et al. Soft X-ray spectrum of a hot plasma. , 1977 .
[50] L. Bildsten. The Fate of Accreted CNO Elements in Neutron Star Atmospheres , 1992 .