Anomalous temporal behaviour of HER X-1

Details Anomalous temporal behaviour of HER X-1 Anomalous temporal behaviour of HER X-1

Aug 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975natur.256..712c&link_type=abstract

Nature, vol. 256, Aug. 28, 1975, p. 712, 713.

Astronomy and Astrophysics

Astronomy

15

Eclipsing Binary Stars, Spaceborne Astronomy, Stellar Radiation, X Ray Sources, Ariel Satellites, Mass Transfer, Neutron Stars, X Ray Spectra

Scientific paper

Counting rate data for 2.4-19.8 keV photons observed by the Ariel V satellite during January 1975 from Her X-1 are reported. An anomalous emission was recorded approximately 16.5 days before the turn on of the source (i.e., during its off state). This observation places a constraint on the mass transfer (from primary star to compact companion) and eclipsing models previously proposed to account for the radiation emitted by Her X-1.

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