NASA NTRS · 19850053279
X-ray emission from Be star binaries
Abstract
A model in which a neutron star in an eccentric inclined orbit around a Be star passes through a ring of matter around the Be star has been used to explain the recurrent flares of X-ray emission from these systems. The optical emission during X-ray flares is due to partial absorption and reprocessing of the X-rays in the ring.
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Apparao, K. M. V.. 1985-05-01. X-ray emission from Be star binaries. https://ntrs.nasa.gov/citations/19850053279
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