VLBI observations of RS CVn and Algol-type binaries

Details VLBI observations of RS CVn and Algol-type binaries VLBI observations of RS CVn and Algol-type binaries

May 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...197..200m&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 197, no. 1-2, May 1988, p. 200-204.

Astronomy and Astrophysics

Astrophysics

24

Cataclysmic Variables, Eclipsing Binary Stars, Peculiar Stars, Very Long Base Interferometry, Astronomical Spectroscopy, Polarization (Waves), Radio Emission, Stellar Magnetic Fields

Scientific paper

The authors report on intercontinental VLBI observations of four RS CVn binaries and of Algol made on 12 June 1986 at λ = 6 cm. All sources were detected at least on the shortest baselines. For one of them (UX Ari) the larger amount of data available allows to conclude that the emission came from an extended, possibly structured region, comparable in size with the binary separation. The authors compare their observations with those obtained previously by Mutel et al. (1985) and discuss briefly the physical implications of these observations for the modelling of radio emission in active late-type binaries.

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