SIMBAD references

1999ApJ...512..892T - Astrophys. J., 512, 892-900 (1999/February-3)

Broadband X-ray spectra of the black hole candidate GRO J1655-40.

TOMSICK J.A., KAARET P., KROEGER R.A. and REMILLARD R.A.

Abstract (from CDS):

We present broadband (2 keV-2 MeV) X-ray spectra of GRO J1655-40, a luminous X-ray transient and occasional source of relativistic radio jets, obtained with the Rossi X-Ray Timing Explorer (RXTE) and the Oriented Scintillation Spectrometer Experiment. In one observation, the luminosity is found to be 18% of the Eddington limit, which is one of the highest luminosities ever observed from GRO J1655-40. For this observation, we find that an adequate fit is obtained when a broad iron line and a reflection component are added to a model consisting of a power law plus a soft excess component. The 95% confidence lower limit on the rms line width is 0.86 keV. The power-law component has a photon index of 2.72+0.03–0.08 and extends to at least 800 keV without a cutoff. After this observation, a significant drop in the (5-12 keV)/(1.5-5 keV) hardness ratio occurred on a timescale less than 2 hr. From an RXTE observation of GRO J1655-40 made after the hardness transition, we find that the power-law index is harder (α=2.415±0.011), the flux of the power-law component is lower, and the total luminosity is 10% of the Eddington limit. The change in the power-law component is consistent with the correlation between the spectral index and power-law flux previously reported for GRO J1655-40.

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Journal keyword(s): Accretion, Accretion Disks - Black Hole Physics - Radiation Mechanisms: Nonthermal - stars: individual (GRO J1655-40) - X-Rays: Stars

Simbad objects: 2

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