Free Access
Issue
Astron. Astrophys. Suppl. Ser.
Volume 128, Number 1, February_II 1998
Page(s) 145 - 151
DOI https://doi.org/10.1051/aas:1998131
Published online 15 February 1998
DOI: 10.1051/aas:1998131

A&A Supplement series, Vol. 128, February II 1998, 145-151

Received June 9, accepted June 20, 1997

X-ray variability of GRS 1915+105 during the low-hard state observed with the Indian X-ray astronomy experiment (IXAE)

B. Paultex2html_wrap518, P.C. Agrawaltex2html_wrap518, A.R. Raotex2html_wrap518, M.N. Vahiatex2html_wrap518, J.S. Yadav tex2html_wrap518, T.M.K. Marartex2html_wrap528, S. Seethatex2html_wrap528, and K. Kasturirangantex2html_wrap528

Send offprint request: B. Paul, bpaul@tifrvax.tifr.res.in

tex2html_wrap534  Tata Institute of Fundamental Research, Homi Bhabha Road, Mumbai 400 005, India
tex2html_wrap536  ISRO Satellite Centre, Airport Road, Vimanpura P.O. Bangalore 560 017, India

Abstract:

The galactic superluminal transient X-ray source GRS 1915+105 was observed with the pointed proportional counters (PPCs) onboard the Indian satellite IRS-P3 during 1996 July 23-27. We report here details of the behavior of this source during the relatively quiet and low luminosity state. Large intensity variations by a factor of 2 to 3, generally seen in black-hole candidates, are observed at a time scale of 100 ms to few seconds. No significant variation is detected over larger time scale of minute or more. The intensity variations are described as sum of shots in the light curve, and the number distribution of the shots are found to be exponential function of the fluence and duration of the shots. The cross correlation spectrum between 6-18  keV and 2-6  keV X-rays is found to have asymmetry signifying a delay of the hard X-rays by about 0.2 to 0.4 s. This supports the idea of hard X-rays being generated by Compton up-scattering from high energy clouds near the source of soft X-rays. Very strong and narrow quasi periodic oscillations in the frequency range 0.62 to 0.82 Hz are observed. We discuss about a model which explains a gradual change in the QPO frequencies with corresponding changes in the mass accretion rate of the disk.

keywords: accretion, accretion disks -- black hole physics -- X-rays: stars -- stars: individual: GRS 1915+105

SIMBAD Objects

Copyright by the European Southern Observatory (ESO)

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.