Centimeter observations of six eclipsing 'Serpentid' binary stars

Details Centimeter observations of six eclipsing 'Serpentid' binary stars Centimeter observations of six eclipsing 'Serpentid' binary stars

Mar 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...352..300e&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 352, March 20, 1990, p. 300-302.

Astronomy and Astrophysics

Astronomy

6

Eclipsing Binary Stars, Radio Astronomy, Stellar Radiation, Centimeter Waves, Emission Spectra, Stellar Luminosity, Synchrotron Radiation

Scientific paper

Centimeter observations of the following eclipsing 'Serpentid' binary stars have been performed: SY And, RX Cas, SX Cas, V367 Cyg, RZ Sct, and W Ser. RZ Sct and W Ser were detected at 3.6 cm, and V367 Cyg was detected at both 6 and 3.6 cm. It is suggested that these objects emit thermalized-gyrosynchrotron radiation as does Beta Lyr but at much lower levels, because the circumstellar environments are different.

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