A VLA survey of nearby flare stars

Details A VLA survey of nearby flare stars A VLA survey of nearby flare stars

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apjs...71..895w&link_type=abstract

Astrophysical Journal Supplement Series (ISSN 0067-0049), vol. 71, Dec. 1989, p. 895-904.

Other

41

Dwarf Stars, Flare Stars, Radio Emission, Very Large Array (Vla), M Stars, Stellar Luminosity, Stellar Spectra, X Ray Spectra

Scientific paper

Results from a VLA survey of nearby flare stars are combined with those of other surveys to compare the incidence of radio detection of late-type dwarf stars with other stellar parameters. About 40 percent of known nearby flare stars were detected in the survey. It is found that there is a deficiency of radio detections for M dwarf stars later than dM5.5, in agreement with the falloff in X-ray luminosity of these stars. Evidence is found for a link between radio activity and rotation, because most of the detected sources are stars which are believed to be young disk stars and are still rapid rotators.

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