A radio detection of V Sagittae

Details A radio detection of V Sagittae A radio detection of V Sagittae

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997mnras.287l..14l&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 287, Issue 3, pp. L14-L16.

Astronomy and Astrophysics

Astronomy

17

Binaries: Close, Stars: Individual: V Sge, Radio Continuum: Stars

Scientific paper

We present a VLA measurement of the peculiar interacting binary V Sge at 3.55 cm. A radio source with flux 70 muJy was detected with 5.4sigma significance <0.1 arcsec from the Carlsberg Meridian Catalogue optical position of V Sge. The probability of an unassociated radio source lying this close to V Sge is extremely low. We use the observed intensity to derive the rate of mass loss from V Sge, and find that it is much greater than that of cataclysmic variables. We discuss the significance of the discovery of this radio emission.

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