Extended emission around the variable radio star LSI +61 deg 303

Details Extended emission around the variable radio star LSI +61 deg 303 Extended emission around the variable radio star LSI +61 deg 303

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987aj.....93.1506f&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 93, June 1987, p. 1506-1510. Research supported by the National Research Council of

Astronomy and Astrophysics

Astronomy

5

Binary Stars, Luminosity, Radio Stars, Stellar Radiation, Variable Stars, Nebulae, Periodic Variations, Relativistic Electron Beams, Supernova Remnants

Scientific paper

Continuum observations of a 2° field at 1420 MHz and a 7.4° field at 408 MHz have been made surrounding the periodic variable radio star LS I +61°303. Extended radio emission was detected around the star. It is proposed that this emission is either (1) thermal gas from the giant H II complex of W3/W4/W5, (2) a supernova remnant whose progenitor is LS I +61°303, or (3) a nonthermal nebula of the type recently discovered around Cir X-1 by Haynes et al. (1986).

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