Please use this identifier to cite or link to this item:
|Title:||Swift observations of MAXI J1659-152: A compact binary with a black hole accretor|
|Authors:||Kennea, J. A.|
Beardmore, A. P.
Evans, P. A.
Curran, P. A.
Krimm, H. A.
Markwardt, C. B.
Krimm, H. A.
|Publisher:||American Astronomical Society (IOP Publishing)|
|Citation:||Astrophysical Journal, 2011, 736 (1), 22|
|Abstract:||We report on the detection and follow-up high-cadence monitoring observations of MAXI J1659–152, a bright Galactic X-ray binary transient with a likely black hole accretor, by Swift over a 27 day period after its initial outburst detection. MAXI J1659–152 was discovered almost simultaneously by Swift and the Monitor of All-sky X-ray Image on 2010 September 25, and was monitored intensively from the early stages of the outburst through the rise to a brightness of ~0.5 Crab by the Swift X-ray, UV/Optical, and the hard X-ray Burst Alert Telescopes. We present temporal and spectral analysis of the Swift observations. The broadband light curves show variability characteristic of black hole candidate transients. We present the evolution of thermal and non-thermal components of the 0.5-150 keV combined X-ray spectra during the outburst. MAXI J1659–152 displays accretion state changes typically associated with black hole binaries, transitioning from its initial detection in the hard state, to the steep power-law state, followed by a slow evolution toward the thermal state, signified by an increasingly dominant thermal component associated with the accretion disk, although this state change did not complete before Swift observations ended. We observe an anti-correlation between the increasing temperature and decreasing radius of the inner edge of the accretion disk, suggesting that the inner edge of the accretion disk infalls toward the black hole as the disk temperature increases. We observed significant evolution in the absorption column during the initial rise of the outburst, with the absorption almost doubling, suggestive of the presence of an evolving wind from the accretion disk. We detect quasi-periodic oscillations that evolve with the outburst, as well as irregular shaped dips that recur with a period of 2.42 ± 0.09 hr, strongly suggesting an orbital period that would make MAXI J1659–152 the shortest period black hole binary yet known.|
|Rights:||Copyright © 2011. The American Astronomical Society. All rights reserved. Deposited with reference to the publisher’s archiving policy available on the SHERPA/RoMEO website.|
|Appears in Collections:||Published Articles, Dept. of Physics and Astronomy|
Files in This Item:
|0004-637X_736_1_22.pdf||Published (publisher PDF)||566.57 kB||Adobe PDF||View/Open|
Items in LRA are protected by copyright, with all rights reserved, unless otherwise indicated.