SUZAKU BROADBAND SPECTROSCOPY OF SWIFT J1753.5-0127 IN THE LOW-HARD STATE
Journal Article
·
· Astrophysical Journal
- Department of Astronomy, University of Michigan, 500 Church Street, Ann Arbor, MI 48109 (United States)
- MIT Kavli Institute for Astrophysics and Space Research, 70 Vasser Street, Cambridge, MA 02139 (United States)
- LAEX, Centro de Astrobiologia (CSIC-INTA), LAEFF, P.O. Box 78, E-28691, Villanueva de la Canada, Madrid (Spain)
We present Suzaku observations of the Galactic black hole candidate Swift J1753.5-0127 in the low-hard state (LHS). The broadband coverage of Suzaku enables us to detect the source over the energy range 0.6-250 keV. The broadband spectrum (2-250 keV) is found to be consistent with a simple power-law (GAMMA approx 1.63). In agreement with previous observations of this system, a significant excess of soft X-ray flux is detected consistent with the presence of a cool accretion disk. Estimates of the disk inner radius infer a value consistent with the innermost stable circular orbit (ISCO; R{sub in} approx< 6R{sub g} , for certain values of, e.g., N{sub H}, i), although we cannot conclusively rule out the presence of an accretion disk truncated at larger radii (R{sub in} approx 10-50R{sub g} ). A weak, relativistically broadened iron line is also detected, in addition to disk reflection at higher energy. However, the iron-K line profile favors an inner radius larger than the ISCO (R{sub in} approx 10-20R{sub g} ). The implications of these observations for models of the accretion flow in the LHS are discussed.
- OSTI ID:
- 21392333
- Journal Information:
- Astrophysical Journal, Journal Name: Astrophysical Journal Journal Issue: 1 Vol. 709; ISSN ASJOAB; ISSN 0004-637X
- Country of Publication:
- United States
- Language:
- English
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