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

We present the results of detailed spectral studies of the ultracompact 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 broadband (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, we find that the two ultracompact LMXBs occupy similar spectral states even though the transitions occur at very different total luminosities.