The three types of high-mass X-ray pulsator

Details The three types of high-mass X-ray pulsator The three types of high-mass X-ray pulsator

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986mnras.220.1047c&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 220, June 15, 1986, p. 1047-1056.

Astronomy and Astrophysics

Astronomy

202

Accretion Disks, Binary Stars, Mass Transfer, Pulsars, Stellar Mass, X Ray Stars, Angular Momentum, B Stars, Orbital Elements, Stellar Envelopes, Stellar Mass Accretion, Stellar Rotation, Supergiant Stars, White Dwarf Stars

Scientific paper

Published observational data on 20 probable high-mass X-ray pulsators are compiled and analyzed. The objects are divided into three classes (those with Be-star primaries, long-pulse-period objects with non-Be-star primaries, and short-period non-Be objects). The implications of the data for mass-transfer processes, spin-period changes, group correlations the questionable classification of A0538-66, and the circumstellar envelopes of Be stars are discussed in detail.

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