RXTE Studies of X-ray Spectral Variations with Accretion Rate in 4U 1915-05

Details RXTE Studies of X-ray Spectral Variations with Accretion Rate in 4U 1915-05 RXTE Studies of X-ray Spectral Variations with Accretion Rate in 4U 1915-05

2000-05-24

arxiv.org/abs/astro-ph/0005497v1

Astronomy and Astrophysics

Astrophysics

27 pages LaTeX, 8 figures, accepted to the Astrophysical Journal

Scientific paper

10.1086/317035

We present the results of detailed spectral studies of the ultra-compact low mass X-ray binary (LMXB) 4U 1915-05 carried out with the Rossi X-ray Timing Explorer (RXTE) during 1996. 4U 1915-05 is an X-ray burster (XRB) known to exhibit a ~199-day modulation in its 2--12 keV flux. Observations were performed with the PCA and HEXTE instruments on RXTE at roughly one-month intervals to sample this long-term period and study accretion rate-related spectral changes. We obtain good fits with a model consisting of a blackbody and an exponentially cut-off power law. The spectral parameters are strongly correlated with both the broad-band (2--50 keV) luminosity and the position in the color-color diagram, with the source moving from a low hard state to a high soft state as the accretion rate increases. The blackbody component appears to drive the spectral evolution. Our results are consistent with a geometry in which the soft component arises from an optically thick boundary layer and the hard component from an extended Comptonizing corona. Comparing our results with those of a similar study of the brighter source 4U 1820-30 (Bloser et al. 2000), we find that the two ultra-compact LMXBs occupy similar spectral states even though the transitions occur at very different total luminosities.

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