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26 April 2024
 
  » arxiv » astro-ph/0105371

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High Frequency Quasi-Periodic Oscillations in the 2000 Outburst of the Galactic Microquasar XTE J1550-564
J. M. Miller ; R. Wijnands ; J. Homan ; T. Belloni ; D. Pooley ; S. Corbel ; C. Kouveliotou ; M. van der Klis ; W. H. G. Lewin ;
Date 22 May 2001
Subject astro-ph
Affiliation MIT Center for Space Research, Univ. of Amsterdam IAP, Oss. Brera, Universite Paris and CEA Saclay, NASA/MSFC
AbstractWe present an analysis of the high frequency timing properties of the April-May 2000 outburst of the black hole candidate and Galactic microquasar XTE J1550-564, measured with the Rossi X-ray Timing Explorer. The rapid X-ray variability we measure is consistent with the source being in either the ``very high’’ or ``intermediate’’ black hole state. Strong (5-8% rms) quasi-periodic oscillations (QPOs) are found between 249-276 Hz; this represents the first detection of the same high frequency QPO in subsequent outbursts of a transient black hole candidate. We also present evidence for lower-frequency QPOs at approximately 188 Hz (3.5 sigma, single trial), also reported previously and likely present simultaneously with the higher-frequency QPOs. We discuss these findings within the context of the 1998 outburst of XTE J1550-564, and comment on implications for models of QPOs, accretion flows, and black hole spin.
Source arXiv, astro-ph/0105371
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