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The 2002 outburst of the microquasar XTE J1550-564

A. P. Colombo·T. Belloni·J. Homan·S. Campana·M. van der Klis
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Abstract

We present results of spectral and timing analysis based on 11 RXTE PCA/HEXTE observations of the microquasar XTE J1550-564 during its last outburst in January 2002. The observed behaviour is comparable to most Black-Hole Candidates in the low/hard state. This is unlike the 1998-99 outburst, when it showed a much more complex feature, probably because of the higher luminosity. For each of the 11 observations we extracted energy spectra and power density spectra, finding typical features of a low/hard state.

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A. P. Colombo, T. Belloni, J. Homan, S. Campana, M. van der Klis. 2002-08-06. The 2002 outburst of the microquasar XTE J1550-564. https://arxiv.org/abs/astro-ph/0208131

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