Observation of hard X-ray flux variability of 3U 0352+30 = X Persei

Details Observation of hard X-ray flux variability of 3U 0352+30 = X Persei Observation of hard X-ray flux variability of 3U 0352+30 = X Persei

Apr 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...229..291f&link_type=abstract

Astrophysical Journal, Part 1, vol. 229, Apr. 1, 1979, p. 291-293.

Astronomy and Astrophysics

Astronomy

10

B Stars, Radiant Flux Density, Variable Stars, X Ray Astronomy, X Ray Stars, Balloon Flight, Energy Spectra, Pressure Distribution

Scientific paper

Two observations of X Per performed on two successive days during the 1976 transatlantic balloon flight show a variation by a factor of 2.6 in the hard X-ray flux of the source. During both observations, corresponding to the transit in the detector field-of-view, the intensity was apparently stable. Comparison with OSO 7 results suggests that the source stays mainly in the state of lower flux.

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