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X-ray Timing Studies of GRS 1915+105

Published online by Cambridge University Press:  25 May 2016

B. Paul ,
P. C. Agrawal ,
A. R. Rao ,
M. N. Vahia ,
J. S. Yadav ,
T. M. K. Marar ,
S. Seetha  and
K. Kasturirangan
B. Paul
Affiliation:
Tata Institute of Fundamental Research Homi Bhaba road, Mumbai (Bombay), 400 005, India
P. C. Agrawal
Affiliation:
Tata Institute of Fundamental Research Homi Bhaba road, Mumbai (Bombay), 400 005, India
A. R. Rao
Affiliation:
Tata Institute of Fundamental Research Homi Bhaba road, Mumbai (Bombay), 400 005, India
M. N. Vahia
Affiliation:
Tata Institute of Fundamental Research Homi Bhaba road, Mumbai (Bombay), 400 005, India
J. S. Yadav
Affiliation:
Tata Institute of Fundamental Research Homi Bhaba road, Mumbai (Bombay), 400 005, India
T. M. K. Marar
Affiliation:
ISRO Satellite Centre, Bangalore, 560 017, India
S. Seetha
Affiliation:
ISRO Satellite Centre, Bangalore, 560 017, India
K. Kasturirangan
Affiliation:
ISRO Satellite Centre, Bangalore, 560 017, India

Extract

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We have made photometric observations of the galactic superluminal jet source GRS 1915+105 in the energy bands of 2-6 and 6-18 keV during 1997 June 12-29 and August 8-10. During our observations, different types of very intense, quasi-regular X-ray bursts have been observed from this source. We present here the light curves and the power density spectra of our observation of this source in its bright state.

Type
Session 3: Diagnostics of High Gravity Objects with X- and Gamma Rays
Information
Symposium - International Astronomical Union , Volume 188: The Hot Universe , 1998 , pp. 394 - 395
Copyright
Copyright © Kluwer 1998