Chandra observations of the neutron star soft X-ray transient RX J170930.2 - 263927 returning to quiescence
暂无分享,去创建一个
P. G. Jonker | G. Nelemans | M. Mendez | G. Nelemans | R. Wijnands | P. Jonker | M. Klis | M. Méndez | M. van der Klis | R. Wijnands | R. Wijnands | Mariano Méndez
[1] J. van Paradijs,et al. Optical and ultraviolet observations of X-ray binaries. , 1995 .
[2] Yasuo Tanaka,et al. ASCA Observations of Transient X-Ray Sources in Quiescence , 1998 .
[3] Space Science Reviews , 1962, Nature.
[4] E. Morgan,et al. The two-hour orbit of a binary millisecond X-ray pulsar , 1998, Nature.
[5] Y. University,et al. A Closer Look at the Soft X-Ray Transient X1608-52: Long-Term Optical and X-Ray Observations , 2001, astro-ph/0112465.
[6] L. Stella,et al. On the Bolometric Quiescent Luminosity and Luminosity Swing of Black Hole Candidate and Neutron Star Low-Mass X-Ray Transients , 2000, astro-ph/0005118.
[7] J. Smak. On the Nature of Dwarf Novae , 1983 .
[8] William E. Harris,et al. A Catalog of Parameters for Globular Clusters in the Milky Way , 1996 .
[9] D. Schlegel,et al. Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds , 1997, astro-ph/9710327.
[10] Deepto Chakrabarty,et al. The Disk-Magnetosphere Interaction in the Accretion-powered Millisecond Pulsar SAX J1808.4–3658 , 1998 .
[11] E. Morgan,et al. The Erratic Luminosity Behavior of SAX J1808.4–3658 during Its 2000 Outburst , 2001, astro-ph/0105446.
[12] M. Livio,et al. The Accretion Disk Limit Cycle Instability in Black Hole X-Ray Binaries , 1995 .
[13] L. Bildsten. The Fate of Accreted CNO Elements in Neutron Star Atmospheres , 1992 .
[14] Martin C. Weisskopf,et al. Astronomy and astrophysics with the advanced X-ray astrophysics facility , 1988 .
[15] Submitted to ApJ Letters , 2002 .
[16] C. Kouveliotou,et al. Chandra Observations of the Anomalous X-Ray Pulsar 1E 2259+586 , 2001, astro-ph/0110182.
[17] C. Sarazin,et al. ROSAT X-Ray Colors and Emission Mechanisms in Early-Type Galaxies , 1998, astro-ph/9804210.
[18] L. Bildsten,et al. Crustal Heating and Quiescent Emission from Transiently Accreting Neutron Stars , 1998, astro-ph/9807179.
[19] Jean H. Swank,et al. The Survey of Low-Mass X-Ray Binaries with the Einstein Observatory Solid-State Spectrometer and Monitor Proportional Counter , 1997 .
[20] G. Nelemans,et al. On the formation of neon-enriched donor stars in ultracompact X-ray binaries , 2002, astro-ph/0204191.
[21] Ramesh Narayan,et al. Advection-dominated Accretion: A Self-similar Solution , 1994 .
[22] J. Zand,et al. Discovery of a Second Millisecond Accreting Pulsar: XTE J1751–305 , 2002, astro-ph/0206491.
[23] X-Ray Spectra from Neutron Stars Accreting at Low Rates , 1994, astro-ph/9407067.
[24] E. Morgan,et al. Discovery of a High-Latitude Accreting Millisecond Pulsar in an Ultracompact Binary , 2002, astro-ph/0206493.
[25] J. Heise,et al. Chandra follow-up of bursters with low persistent emission , 2002, astro-ph/0207138.
[26] Robert E. Rutledge,et al. Variable Thermal Emission from Aquila X-1 in Quiescence , 2002, astro-ph/0204196.
[27] G. Pavlov,et al. Spectra of X-ray bursts at near-Eddington luminosities , 1991 .
[28] D. Schlegel,et al. Maps of Dust Infrared Emission for Use in Estimation of Reddening and Cosmic Microwave Background Radiation Foregrounds , 1998 .
[29] Chandra Observations of the Bursting X-Ray Transient SAX J1747.0–2853 during Low-Level Accretion Activity , 2002, astro-ph/0202151.
[30] 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.
[31] M. Colpi,et al. Charting the Temperature of the Hot Neutron Star in a Soft X-Ray Transient , 2000, astro-ph/0010572.
[32] A. King. The population of faint transients in the Galactic Centre , 2000, astro-ph/0004277.
[33] M. Colpi,et al. An XMM-Newton Study of the 401 Hz Accreting Pulsar SAX J1808.4–3658 in Quiescence , 2002, astro-ph/0206376.
[34] S. Campana,et al. The neutron stars of Soft X–ray Transients , 1993, astro-ph/9805079.
[35] Paul S. Smith,et al. The optical polarization properties of X-ray-selected BL Lacertae objects , 1994 .
[36] R. Wijnands,et al. A millisecond pulsar in an X-ray binary system , 1998, Nature.
[37] Walter H. G. Lewin,et al. X-ray binaries. , 1976 .
[38] D. Christian,et al. Accretion Disk Corona Line Emission from X0614+091 , 1994 .
[39] J. van Paradijs,et al. On the Accretion Instability in Soft X-Ray Transients , 1996 .
[40] R. Wijnands,et al. XMM-Newton Spectroscopy of the Accretion-driven Millisecond X-Ray Pulsar XTE J1751–305 in Outburst , 2002, astro-ph/0208166.
[41] G. Basri,et al. Dynamic Processes in Be Star Atmospheres. IV. Common Attributes of Line Profile ``Dimples'' , 1996 .
[42] F. Paerels,et al. Neon Line Emission in the X-Ray Spectrum of the Pulsar 4U 1626–67 , 1995 .
[43] Yasuo Tanaka,et al. X-ray novae , 1996 .
[44] Mario Livio,et al. The Properties of X-Ray and Optical Light Curves of X-Ray Novae , 1997 .
[45] J. Lasota. The disc instability model of dwarf novae and low-mass X-ray binary transients , 2001, astro-ph/0102072.
[46] J. Dickey,et al. H I in the Galaxy , 1990 .