Observations of the X ray pulsars from the KVANT module

Details Observations of the X ray pulsars from the KVANT module Observations of the X ray pulsars from the KVANT module

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.296...71g&link_type=abstract

In ESA, The 23rd ESLAB Symposium on Two Topics in X Ray Astronomy. Volume 1: X Ray Binaries p 71-79 (SEE N90-25711 19-89)

Astronomy and Astrophysics

Astronomy

4

Mir Space Station, Pulsars, Radio Bursts, X Ray Spectra, Center Of Gravity, Data Acquisition, Satellite Observation, Stellar Spectra, X Ray Binaries

Scientific paper

The results of observations of the following X-ray pulsars are discussed: Cen X-3, SMCX-1, Her X-1, Vela X-1, A0535+26, 4U 1626-67 and GX 1+4. The observations were performed by the instruments onboard Kvant module from 1987 to 1989. The pulsation period measurements are presented and the values of the periods are reduced to the solar system baricenter and (except in the case of A0535+26 and 4U 1626-67) to the binary system baricenter.

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