The X-ray behaviour of 3U 0352+30 (X Per)

Details The X-ray behaviour of 3U 0352+30 (X Per) The X-ray behaviour of 3U 0352+30 (X Per)

Jul 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976mnras.176..201w&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 176, July 1976, p. 201-215. Research supported by the Science Research

Astronomy and Astrophysics

Astronomy

92

Satellite-Borne Instruments, Stellar Spectra, Time Response, X Ray Sources, Ariel Satellites, B Stars, Graphs (Charts), Oao 3, Power Spectra

Scientific paper

A series of observations of the X-ray source 3U 0352+30 made with the Copernicus and Ariel 5 satellites is reported. Evidence is found for 13.9-min and 22-hr modulations of the X-ray flux. The data also indicate long- and short-term changes in the slope of the X-ray spectrum and the amount of low-energy absorption. The implications of these results are discussed, especially for the proposed identification of the X-ray source with X Per.

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