Rapid X-ray variability in GRO J0422+32 (Nova Per 1992)

Details Rapid X-ray variability in GRO J0422+32 (Nova Per 1992) Rapid X-ray variability in GRO J0422+32 (Nova Per 1992)

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..410..947v&link_type=abstract

The fourth compton symposium. AIP Conference Proceedings, Volume 410, pp. 947-951 (1997).

Computer Science

Gamma-Ray Sources, Gamma-Ray Bursts, Gamma-Ray

Scientific paper

We present the results of an analysis of the time variability of the soft X-ray transient GRO J0422+32 (Nova Per 1992) observed with BATSE. Our analysis covers the entire ~200 day outburst, beginning with the first detection of the source on 1992 August 5. We obtained power density spectra (PDS) in the 20-100 keV energy band covering the frequency interval 0.002-0.488 Hz. The PDSs of GRO J0422+32 show a peak of quasi-periodic oscillations (QPOs) with a centroid frequency of ~200 mHz, during the first 120 days of the outburst.

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