Non-Canonical Insights into the Evolution of Stars. 1. an Alternative Model of Massive X-Ray Binaries

Details Non-Canonical Insights into the Evolution of Stars. 1. an Alternative Model of Massive X-Ray Binaries Non-Canonical Insights into the Evolution of Stars. 1. an Alternative Model of Massive X-Ray Binaries

Nov 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985baicz..36..327h&link_type=abstract

Bulletin of the Astronomical Institute of Czechoslovakia, vol. 36, p.327

Astronomy and Astrophysics

Astronomy

17

Scientific paper

Observational data on known massive X-ray binaries have been collected and critically examined. It is concluded that the mass transfer in these systems proceeds basically from the X-ray secondaries to the optical primaries, not in the opposite direction as usually believed. The X-ray components of these systems are not neutron stars or black holes, but rotationally unstable compact helium stars contracting after the end of case B of mass exchange.

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