The peak radio emission phase variations in the Be-star/X-ray source LSI+61degr 303

Details The peak radio emission phase variations in the Be-star/X-ray source LSI+61degr 303 The peak radio emission phase variations in the Be-star/X-ray source LSI+61degr 303

Nov 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999a%26a...351..551a&link_type=abstract

Astronomy and Astrophysics, v.351, p.551-553 (1999)

Astronomy and Astrophysics

Astrophysics

3

Accretion, Accretion Disks, Stars: Binaries: General, Stars: Emission-Line, Be, Stars: Individual: Lsi +61Deg 303, Radio Continuum: Stars, X-Rays: Stars

Scientific paper

The orbital phase of the peak radio emission in the Be star/X-ray source LSI +61degr 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.

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