INTEGRAL observations of the black hole candidate H 1743-322 in outburst
arXiv:astro-ph/0307474 · doi:10.1051/0004-6361:20031140
Abstract
INTEGRAL made 3 observations in 2003 April of the black hole candidate H 1743-322 during the rising part, and close to the maximum, of an outburst. H 1743-322 was previously observed in outburst in 1977-1978. The source is located in a crowded region of the sky (l = 357 deg, b = -2 deg) and at least 18 sources are clearly detected in the field of view of the gamma-ray imager during a 277 ksec exposure. These are well known persistent X-ray binaries and 3 transient sources in outburst. The combined 5-200 keV JEM-X and SPI spectrum of H 1743-322 is well fit with an absorbed ((2.5 10E22 atom/cm2) soft (photon index 2.70 +/- 0.09) power-law model consistent with J 1743-322 being in a high/soft state.
arXiv comment5 pages. Figs. 2 and 3 are best viewed in color. To appear in INTEGRAL special edition of A&AL
References in corpus (4)
Cited by in corpus (25)
- Radiatively efficient accreting black holes in the hard state: the case study of H1743-322
- High- and low-frequency quasi-periodic oscillations in the X-ray light curves of the black hole transient H1743-322
- The 2003 Outburst of the X-ray Transient H 1743-322: Comparisons with the Black Hole Microquasar XTE J1550-564
- A failed outburst of H1743-322
- The INTEGRAL Galactic bulge monitoring program: the first 1.5 years
- A Model for the Correlation of Hard X-ray Index with Eddington Ratio in Black Hole X-ray Binaries
- The Galactic black hole transient H1743-322 during outburst decay: connections between timing noise, state transitions and radio emission
- Evolution of the temporal and the spectral properties in 2010 and 2011 outbursts of H 1743-322
- INTEGRAL observations of five sources in the Galactic Center region
- The 2004 Outburst of BHC H1743-322: Analysis of spectral and timing properties using the TCAF Solution
- High-energy observations of the state transition of the X-ray nova and black hole candidate XTE J1720-318
- 1E 1740.7-2942: temporal and spectral evolution from INTEGRAL and RXTE observations
- The INTEGRAL view on Black Hole X-ray Binaries
- 3-200 keV spectral states and variability of the INTEGRAL Black Hole binary IGR J17464-3213
- Delayed Outburst of H 1743--322 in 2003 and relation with its other outbursts
- State transition and flaring activity of IGR J17464-3213/H1743-322 with SPI/INTEGRAL telescope
- The early phase of a H1743-322 outburst observed by INTEGRAL, RXTE, Swift, and XMM/Newton
- The 2009 outburst of H~1743-322 as observed by RXTE
- Using XMM-Newton to study the energy dependent variability of H 1743-322 during its 2014 outburst
- 2016 outburst of H~1743--322: \textit{XMM-Newton} and \textit{NuSTAR} view
- Trace the Accretion Geometry of H 1743--322 with Type C Quasi-periodic Oscillations in Multiple Outbursts
- Testing the dynamic origin of Quasi-periodic Oscillations in MAXI J1535-571 and H 1743-322
- Infrared study of H1743-322 in outburst: a radio-quiet and NIR-dim microquasar
- No X-Ray Excess from the HESS J1741-302 Region except a New Intermediate Polar Candidate
- AstroSat Observation of 2016 Outburst of H 1743-322