X-ray variability of the AM HER star CW1103 + 254

Details X-ray variability of the AM HER star CW1103 + 254 X-ray variability of the AM HER star CW1103 + 254

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ssrv...40..139b&link_type=abstract

(ESA, ESLAB Symposium on X-Ray Astronomy in the EXOSAT Era, 18th, The Hague, Netherlands, Nov. 5-9, 1984) Space Science Reviews

Astronomy and Astrophysics

Astronomy

8

Stellar Spectrophotometry, Variable Stars, X Ray Sources, Emission Spectra, Exosat Satellite, Light Curve, Periodic Variations, Spectral Energy Distribution, Temporal Distribution

Scientific paper

The AM Her star CW1103+254 was observed with the low-energy and the
medium-energy instruments of EXOSAT on 3 occasions for a total of 10.5
orbital cycles. Both, soft and hard X-rays from CW1103+254 were
detected. The authors report preliminary results on the time variability
of the X-ray emission on time scales from 1 minute to 1 month.

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