The results of X-ray observations of Galactic superluminal jet source GRS 1
915 + 105 during its low luminosity state and state transitions in October,
1996 - April, 1997 with PCA and HEXTE instruments aboard RXTE are reported
.
Except some peculiarities, the major spectral and temporal properties of th
e source during this period were similar to that of the Galactic black hole
candidates in the intermediate state (corresponding to the transition betw
een the canonical high and low states). The power law component of the spec
trum 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 p
ower density spectrum in this state. The changes of the QPO centroid freque
ncy are strongly correlated with the changes of spectral and timing paramet
ers (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 repo
rted period) they would match the canonical values for a low state of the G
alactic black hole candidates.