Evidence for extended radio emission surrounding RX Puppis

Details Evidence for extended radio emission surrounding RX Puppis Evidence for extended radio emission surrounding RX Puppis

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986apj...301..877h&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 301, Feb. 15, 1986, p. 877-880.

Astronomy and Astrophysics

Astronomy

15

Radio Emission, Radio Sources (Astronomy), Stellar Mass Ejection, Stellar Radiation, Stellar Winds, Symbiotic Stars, Hot Stars, Least Squares Method, Radio Astronomy

Scientific paper

Evidence for an approximately 1-arcsec extended structure in 6 cm continuum emission emanating from the symbiotic star system RX Puppis is reported. Hourly continuum flux changes were not detected as suggested in previous radio experiments by others. The observations indicate that the predominant nature of the radio emission is thermal and consistent with an optically thick stellar wind emanating from the symbiotic star system. The results presented here are discussed with regard to other similar stellar binary systems.

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