Swift observations of MAXI J1659-152: A compact binary with a black hole accretor

Jamie A. Kennea, P. Romano, V. Mangano, A. P. Beardmore, P. A. Evans, P. A. Curran, H. A. Krimm, C. B. Markwardt, K. Yamaoka

Research output: Contribution to journalArticle

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Abstract

We report on the detection and follow-up high-cadence monitoring observations of MAXIJ1659-152, a bright Galactic X-ray binary transient with a likely black hole accretor, by Swift over a 27day period after its initial outburst detection. MAXIJ1659-152 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 ∼0.5Crab 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 0.5-150keV combined X-ray spectra during the outburst. MAXIJ1659-152 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 ± 0.09hr, strongly suggesting an orbital period that would make MAXIJ1659-152 the shortest period black hole binary yet known.

Original languageEnglish (US)
Article number22
JournalAstrophysical Journal
Volume736
Issue number1
DOIs
StatePublished - Jul 20 2011

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outburst
accretion disks
accretion
x rays
temporal analysis
spectral analysis
light curve
spectrum analysis
sky
monitors
dip
bursts
power law
brightness
temperature
oscillation
telescopes
broadband
orbitals
oscillations

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Kennea, J. A., Romano, P., Mangano, V., Beardmore, A. P., Evans, P. A., Curran, P. A., ... Yamaoka, K. (2011). Swift observations of MAXI J1659-152: A compact binary with a black hole accretor. Astrophysical Journal, 736(1), [22]. https://doi.org/10.1088/0004-637X/736/1/22
Kennea, Jamie A. ; Romano, P. ; Mangano, V. ; Beardmore, A. P. ; Evans, P. A. ; Curran, P. A. ; Krimm, H. A. ; Markwardt, C. B. ; Yamaoka, K. / Swift observations of MAXI J1659-152 : A compact binary with a black hole accretor. In: Astrophysical Journal. 2011 ; Vol. 736, No. 1.
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Kennea, JA, Romano, P, Mangano, V, Beardmore, AP, Evans, PA, Curran, PA, Krimm, HA, Markwardt, CB & Yamaoka, K 2011, 'Swift observations of MAXI J1659-152: A compact binary with a black hole accretor', Astrophysical Journal, vol. 736, no. 1, 22. https://doi.org/10.1088/0004-637X/736/1/22

Swift observations of MAXI J1659-152 : A compact binary with a black hole accretor. / Kennea, Jamie A.; Romano, P.; Mangano, V.; Beardmore, A. P.; Evans, P. A.; Curran, P. A.; Krimm, H. A.; Markwardt, C. B.; Yamaoka, K.

In: Astrophysical Journal, Vol. 736, No. 1, 22, 20.07.2011.

Research output: Contribution to journalArticle

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