On the nature of low-luminosity Be/X ray binaries

Details On the nature of low-luminosity Be/X ray binaries On the nature of low-luminosity Be/X ray binaries

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.296..583p&link_type=abstract

In ESA, The 23rd ESLAB Symposium on Two Topics in X Ray Astronomy. Volume 1: X Ray Binaries p 583 (SEE N90-25711 19-89)

Computer Science

Performance

Rosat Mission, Stellar Evolution, Stellar Luminosity, X Ray Binaries, B Stars, Performance Prediction, Spectrum Analysis, Stellar Spectra, Variable Stars, White Dwarf Stars, X Ray Astronomy

Scientific paper

The existence of a class of low luminosity X ray sources, consisting of
a Be star and a white dwarf, is proposed. ROSAT is expected to discover
several dozen of these systems. They are expected to outnumber the
classical Be/X ray binaries by a factor of about 10.

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