On the hard, pulsating X-ray transients.

Details On the hard, pulsating X-ray transients. On the hard, pulsating X-ray transients.

Nov 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990rmxaa..21..467j&link_type=abstract

Revista Mexicana de Astronomia y Astrofisica, Vol. 21, p. 467 - 470

Astronomy and Astrophysics

Astronomy

X-Ray Transients: Be Stars, X-Ray Transients: Accretion

Scientific paper

It is shown that the X-ray luminosities observed in Be/X-ray systems can
be explained by accretion from the extended, equatorially-concentrated,
expanding envelope of the Be companion.

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