1996/1997 low luminosity state and state transitions of GRS1915+105: RXTE observations

Details 1996/1997 low luminosity state and state transitions of GRS1915+105: RXTE observations 1996/1997 low luminosity state and state transitions of GRS1915+105: RXTE observations

1998-11-27

arxiv.org/abs/astro-ph/9811449v1

Astron. Lett., 25, 827, 1999

Astronomy and Astrophysics

Astrophysics

34 pages, 14 figures. Submitted to Astronomy Letters

Scientific paper

The results of X-ray observations of Galactic superluminal jet source GRS 1915+105 during its low luminosity state and state transitions in October, 1996 - April, 1997 with PCA and HEXTE instruments aboard Rossi X-ray Timing Explorer (RXTE) are reported. Except some peculiarities, the major spectral and temporal properties of the source during this period were similar to that of the Galactic black hole candidates in the intermediate state (corresponding to the transition between the canonical high and low states). The power law component of the spectrum gradually hardens with decrease of the source flux in the 3 - 150 keV energy band. The 2 - 10 Hz QPOs were found to be a generic feature of the power density spectrum in this state. The changes of the QPO centroid frequency are strongly correlated with the changes of spectral and timing parameters (in particular parameters of the soft spectral component). This type of correlation holds on the wide range of time scales (from seconds to months). Overall trend of the spectral and temporal properties suggests that with further drop of the source flux (below the values observed during the reported period) they would match the canonical values for a low state of the Galactic black hole candidates.

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