Astronomy and Astrophysics – Astrophysics
Scientific paper
1996-03-27
Astronomy and Astrophysics
Astrophysics
15 pages, 4 Postscript figures, uses aasms4.sty. Accepted for publication in Astrophysical Journal Letters
Scientific paper
10.1086/310063
We have examined fifteen days of CGRO/BATSE data, obtained during the first outburst of the black-hole candidate source GRO J1655-40, to search for rapid variability of its X-ray flux. We find no evidence for significant variability of GRO J1655-40 during our observations, with a 2 sigma upper limit to the fractional r.m.s. amplitude in the frequency range 0.03-0.488 Hz of 6.6%. We cannot, on the basis of our observations, determine the source state (low, high, or very-high state) of GRO J1655-40.
Crary David J.
der Hooft Frank van
Finger Mark H.
Harmon Alan B.
Kouveliotou Chryssa
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