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1999A&A...351..551A - Astronomy and Astrophysics, volume 351, 551-553 (1999/11-2)
The peak radio emission phase variations in the Be-star/X-ray source LSI+61 303.
APPARAO K.M.V.
Abstract (from CDS):
The orbital phase of the peak radio emission in the Be star/X-ray source LSI +61 303 shows variations ranging from 0.5 to 0.9, the weaker emissions showing the larger phase. The delay in attaining peak emission is explained as due to the time required for the relativistic gas bubble responsible for the radio emission, expanding in the hot wind of the Be star, to become large enough in size to become optically thin at the radio frequencies.
Abstract Copyright: ∼
Journal keyword(s): accretion, accretion disks - stars: binaries: general - stars: emission-line, Be - stars: individual: LSI +61 303 - radio continuum: stars - X-rays: stars
Simbad objects: 1
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