X ray observations of GS2023+338 by the KVANT module

Details X ray observations of GS2023+338 by the KVANT module X ray observations of GS2023+338 by the KVANT module

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.296..255a&link_type=abstract

In ESA, The 23rd ESLAB Symposium on Two Topics in X Ray Astronomy. Volume 1: X Ray Binaries p 255-261 (SEE N90-25711 19-89)

Astronomy and Astrophysics

Astronomy

2

Noise Spectra, Power Spectra, X Ray Astronomy, X Ray Sources, X Ray Spectra, Mir Space Station, Spaceborne Experiments, Stellar Luminosity, Stellar Parallax, X Ray Spectroscopy, X Ray Timing Explorer

Scientific paper

Following the discovery of GS2023+338 by Ginga, the source was detected in the 2 to 300 keV energy band by the experiments onboard the Kvant module. The source position was localized using data from the coded mask imaging spectrometer. Between Jun. 8 to Aug. 1989 a continuous decrease of X-ray luminosity and strong short time variability were detected. Timing analysis showed strong low frequency noise in the power spectrum of the source.

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