Variability of GX3 + 1 observed with EXOSAT

Details Variability of GX3 + 1 observed with EXOSAT Variability of GX3 + 1 observed with EXOSAT

Apr 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ncimc..13..463d&link_type=abstract

Nuovo Cimento C, Serie 1 (ISSN 0390-5551), vol. 13 C, Mar.-Apr. 1990, p. 463-469. Research supported by CNR.

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Exosat Satellite, X Ray Sources, Low Frequencies, Periodic Variations, Random Noise

Scientific paper

Results from an observation of the X-ray source GX3 + 1 carried out with the Exosat satellite on October 23, 1983, are reported. The source showed a strong X-ray variability in excess of the counting statistics noise. This variability increased toward low frequencies (red noise) and was different in different energy bands, with the lower energy X-rays showing a more pronounced increase of the variability at low frequencies. The variation function of the source is also shown to depend on energy, with the highest values associated with the highest energies. A comparison of the time variability properties of GX3 + 1 with those of other bright low mass X-ray binaries is presented.

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