Tools
Sorted by:
Try your query at:
 |
 |
 |
 |
 |
 |
Results 1 - 10
of
182
X-ray Nova XTE J1550-564: RXTE Spectral Observations
, 1999
"... Excellent coverage of the 1998 outburst of the X-ray Nova XTE J1550–564 was provided by the Rossi X-ray Timing Explorer. XTE J1550–564 exhibited an intense (6.8 Crab) flare on 1998 September 19 (UT), making it the brightest new X-ray source observed with RXTE. We present a spectral analysis utilizin ..."
Abstract
- Add to MetaCart
canonical outburst states of Black Hole X-ray Novae. Subject headings: black hole physics — stars: individual (XTE J1550-564) — X-rays: stars – 3 – 1.
INTEGRAL and XMM-Newton spectroscopy of GX 339–4 during Hard/Soft Intermediate and High/Soft States in the 2007
, 810
"... outburst ..."
A failed outburst of H1743-322
- MNRAS
, 2009
"... We report on a campaign of X-ray and soft γ-ray observations of the black hole candidate (BHC) H1743−322 (also named IGR J17464-3213), performed with the RXTE, INTEGRAL and Swift satellites. The source was observed during a short outburst between 2008 October 03 and November 16. The evolution of the ..."
Abstract
-
Cited by 1 (0 self)
- Add to MetaCart
of the hardness–intensity diagram throughout the outburst is peculiar, in that it does not follow the canonical pattern through all the spectral states (the so-called q-track pattern) seen during the outburst of black hole transients. On the contrary, the source only makes a transition from the hard state
“Canonical ” Black Hole States in the Superluminal Source GRO J1655–40
, 1998
"... We analyze RXTE/PCA observations of the black hole candidate and galactic superluminal source GRO J1655–40 during its recent outburst. We show that during its decay to quiescence, GRO J1655–40 goes through the high, intermediate, and low state (and that at the beginning of its decay it might have ev ..."
Abstract
- Add to MetaCart
We analyze RXTE/PCA observations of the black hole candidate and galactic superluminal source GRO J1655–40 during its recent outburst. We show that during its decay to quiescence, GRO J1655–40 goes through the high, intermediate, and low state (and that at the beginning of its decay it might have
Phototmetry of V1062 Tau: low states, short outbursts, and period-switching
, 2004
"... Intermediate polars (IPs) are a subclass of Cataclysmic Variables (CVs) having a white dwarf, the magnetic field of which is strong enough to control (at least partially) the accretion flow from the secondary star, but is not strong ..."
Abstract
-
Cited by 1 (0 self)
- Add to MetaCart
Intermediate polars (IPs) are a subclass of Cataclysmic Variables (CVs) having a white dwarf, the magnetic field of which is strong enough to control (at least partially) the accretion flow from the secondary star, but is not strong
The Evolution of Disks and Winds in Dwarf Novae Outbursts
, 2001
"... Abstract. Far ultraviolet (FUV) observations are excellent probes of the inner accretion disk, disk outflows, and the mass-accumulating white dwarf in cataclysmic variables. Here we study the contrasting behavior of two canonical dwarf novae in outburst by presenting FUSE FUV (904 – 1187 ˚A) spectro ..."
Abstract
- Add to MetaCart
Abstract. Far ultraviolet (FUV) observations are excellent probes of the inner accretion disk, disk outflows, and the mass-accumulating white dwarf in cataclysmic variables. Here we study the contrasting behavior of two canonical dwarf novae in outburst by presenting FUSE FUV (904 – 1187 ˚A
Evolution of Spectral States of Aql X-1 during the 2000 Outburst
, 2004
"... We present the results of detailed analysis of X-ray data in 3-20 keV range from a ∼ 70 day outburst of the neutron star transient Aquila X-1 during September-November 2000. Optical monitoring with the YALO 1m telescope was used to trigger X-ray observations with Rossi X-ray Timing Explorer (RXTE) i ..."
Abstract
- Add to MetaCart
) in order to follow the outburst from a very early stage. In this paper we discuss the correlated evolution in time of features in the spectral and temporal domains, for the entire outburst. The state transition from low/hard state to high/soft state during the rise of the outburst occurs at higher
“Soft X-ray transient ” outbursts which aren’t soft
, 2003
"... We have accumulated multiwavelength (X-ray, optical, radio) lightcurves for the eight black hole X-ray binaries which have been observed to enter a supposed ‘soft X-ray transient ’ outburst, but remained in the low/hard state throughout the outburst. Comparison of the lightcurve morphologies, spectr ..."
Abstract
-
Cited by 1 (0 self)
- Add to MetaCart
We have accumulated multiwavelength (X-ray, optical, radio) lightcurves for the eight black hole X-ray binaries which have been observed to enter a supposed ‘soft X-ray transient ’ outburst, but remained in the low/hard state throughout the outburst. Comparison of the lightcurve morphologies
RXTE Observations of XTE J1550–564 during its 2000 outburst
, 2002
"... We report on timing and spectral observations of the microquasar XTE J1550−564 during its 2000 outburst made by the Rossi X-ray Timing Experiment (RXTE). We study the spectral properties of the source during both the rise to the outburst and its decline. We observe transitions from a low hard state ..."
Abstract
- Add to MetaCart
We report on timing and spectral observations of the microquasar XTE J1550−564 during its 2000 outburst made by the Rossi X-ray Timing Experiment (RXTE). We study the spectral properties of the source during both the rise to the outburst and its decline. We observe transitions from a low hard state
Results 1 - 10
of
182
