Radio emission from RSCVn stars, Algol, and LSI+61 deg 303

Details Radio emission from RSCVn stars, Algol, and LSI+61 deg 303 Radio emission from RSCVn stars, Algol, and LSI+61 deg 303

Feb 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...268..178e&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 268, no. 1, p. 178-182.

Astronomy and Astrophysics

Astrophysics

11

Radio Emission, Stellar Systems, X Ray Binaries, Astronomical Polarimetry, Spectral Emission, Stellar Flares

Scientific paper

Multiepoch radio observations at 8.4 GHz (3.6 cm wavelength) of 19 RSCVn stars, Algol, and LSI+61 deg 303 are reported. For the UX Ari system, we have observed a series of flares with a moderate emission level. Their emission was partly circularly polarized and the sense of the polarization was the same as in observations carried out, at the same frequency, three years before. The radio periodic X-ray binary LSI+61 deg 303 has been observed for a full period. The outburst peak flux density suggests a value for the four-year modulation period slightly greater than previously reported.

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