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Results 11 - 20
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496
The properties of X-ray and optical light curves of X-ray novae
- Phys. Rev. 59:539– Gnedin OY, Yakovlev DG, Potekhin AY. 2001. Thermal relaxation in young neutron
, 1997
"... We have collected the available data from the literature and from public data archives covering the past two decades for the long-term X-ray and optical light curves of X-ray nova (XN) outbursts. XN outbursts are due to episodic accretion events, primarily in low-mass X-ray binaries normally charact ..."
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Cited by 11 (0 self)
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We have collected the available data from the literature and from public data archives covering the past two decades for the long-term X-ray and optical light curves of X-ray nova (XN) outbursts. XN outbursts are due to episodic accretion events, primarily in low-mass X-ray binaries normally
ADVECTION-DOMINATED ACCRETION MODEL OF X-RAY NOVA MUSCAE IN OUTBURST
, 1997
"... We present a model for the high-low state transition of the X-Ray Nova GS 1124-68 (Nova Muscae 1991) observed by Ginga 1. The model consists of an advectiondominated accretion flow (ADAF) near the central black hole surrounded by a thin accretion disk. During the rise phase of the outburst, as the m ..."
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We present a model for the high-low state transition of the X-Ray Nova GS 1124-68 (Nova Muscae 1991) observed by Ginga 1. The model consists of an advectiondominated accretion flow (ADAF) near the central black hole surrounded by a thin accretion disk. During the rise phase of the outburst
Resolved Jets and Long-Period Black Hole X-ray Novae
, 2003
"... In this brief note we point out that the four spatially resolved relativistic jets among the 14 dynamically confirmed black hole X-ray novae are all in systems with long orbital periods. Many shorter period systems show transient radio outbursts which are attributed to jets, but these jets have not ..."
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In this brief note we point out that the four spatially resolved relativistic jets among the 14 dynamically confirmed black hole X-ray novae are all in systems with long orbital periods. Many shorter period systems show transient radio outbursts which are attributed to jets, but these jets have
Characterizing the QPO Behavior of the X-ray Nova XTE J1550–564
, 1999
"... For all 209 RXTE observations of the X-ray nova XTE J1550–564 during its major outburst of 1998-1999, we have analyzed the X-ray power spectra, phase lags, and coherence functions. These observations constitute one of the richest and most complete data sets obtained for any black hole X-ray nova. Th ..."
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For all 209 RXTE observations of the X-ray nova XTE J1550–564 during its major outburst of 1998-1999, we have analyzed the X-ray power spectra, phase lags, and coherence functions. These observations constitute one of the richest and most complete data sets obtained for any black hole X-ray nova
Rotational Broadening and Doppler Tomography of the Quiescent X-Ray Nova Centaurus X-4
, 2008
"... X-ray novae (XRNe) are a subclass of low mass X-ray binaries characterized by the exhibition of occasional outbursts with a recurrence time-scale of a few decades (see the reviews ..."
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X-ray novae (XRNe) are a subclass of low mass X-ray binaries characterized by the exhibition of occasional outbursts with a recurrence time-scale of a few decades (see the reviews
Modeling of non-stationary accretion disks in X-ray novae A 0620−00 and GRS 1124−68 during outburst
, 805
"... Received xxx/Accepted xxx Aims. We address the task of modeling soft X-ray and optical light curves of X-ray novae in the high/soft state. Methods. The analytic model of viscous evolution of an externally truncated accretionα-disk is used. Relativistic effects near a Kerr black hole and self-irradia ..."
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Received xxx/Accepted xxx Aims. We address the task of modeling soft X-ray and optical light curves of X-ray novae in the high/soft state. Methods. The analytic model of viscous evolution of an externally truncated accretionα-disk is used. Relativistic effects near a Kerr black hole and self
RXTE broad band observations of X-ray Nova XTE J1755-324
"... . The properties of X-ray Nova XTE J1755--324, observed with RXTE observatory in 1997 are reported. The lightcurve of the source was typical for X-ray Novae, except for somewhat shorter decay time scale and the time elapsed between the primary and subsequent secondary and tertiary outbursts. At the ..."
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. The properties of X-ray Nova XTE J1755--324, observed with RXTE observatory in 1997 are reported. The lightcurve of the source was typical for X-ray Novae, except for somewhat shorter decay time scale and the time elapsed between the primary and subsequent secondary and tertiary outbursts
Characterizing the Low-Frequency QPO behavior of the X-ray Nova XTE J1550–564
, 2000
"... For all 209 RXTE observations of the 7-Crab X-ray nova XTE J1550–564, we analyzed the X-ray power spectra, phase lags, and coherence functions. These observations cover the entire 250 day outburst cycle of the source and are the most complete and arguably the richest data set for any black hole X-ra ..."
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For all 209 RXTE observations of the 7-Crab X-ray nova XTE J1550–564, we analyzed the X-ray power spectra, phase lags, and coherence functions. These observations cover the entire 250 day outburst cycle of the source and are the most complete and arguably the richest data set for any black hole X-ray
The outburst radial velocity curve of X-ray Nova Scorpii 1994 (=GRO J165540): a reduced mass for the black hole
- MNRAS
, 1999
"... X-ray novae are low-mass binary systems in which a compact object undergoes unstable accretion from a late-type companion star, releasing energy in the form of X-rays. In a ..."
Abstract
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Cited by 2 (0 self)
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X-ray novae are low-mass binary systems in which a compact object undergoes unstable accretion from a late-type companion star, releasing energy in the form of X-rays. In a
RXTE Observations of an Outburst of Recurrent X-ray Nova GS 1354–644
, 1999
"... We present the results of Rossi X-ray Timing Explorer observations of GS 1354–644 during a modest outburst in 1997-1998. The source is one of a handful of black hole X-ray transients that are confirmed to be recurrent in X-rays. A 1987 outburst of the same source observed by Ginga was much brighter, ..."
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We present the results of Rossi X-ray Timing Explorer observations of GS 1354–644 during a modest outburst in 1997-1998. The source is one of a handful of black hole X-ray transients that are confirmed to be recurrent in X-rays. A 1987 outburst of the same source observed by Ginga was much brighter
Results 11 - 20
of
496
