On the spin down episodes of VELA X-1

Details On the spin down episodes of VELA X-1 On the spin down episodes of VELA X-1

Jul 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...111..365m&link_type=abstract

Astronomy and Astrophysics, vol. 111, no. 2, July 1982, p. 365-367.

Astronomy and Astrophysics

Astronomy

12

Binary Stars, Stellar Mass Accretion, Stellar Rotation, X Ray Sources, Cos-B Satellite, Neutron Stars, X Ray Astronomy

Scientific paper

The ESA COS-B satellite observed the X-ray source Vela X-1 in
July/August 1976 and in October/November 1979 in the energy range 2-12
keV. Different pulse periods, 282.819 and 282.782 s, were determined for
the two observations respectively. These values confirm the presence of
spin up and spin down processes in this source.

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