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- W3104393968 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." @default.
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- W3104393968 date "1985-01-01" @default.
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- W3104393968 title "X-ray emission from Be star binaries." @default.
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