Flare activity of Proxima Centauri

Details Flare activity of Proxima Centauri Flare activity of Proxima Centauri

Jun 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981mnras.195.1029w&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 195, June 1981, p. 1029-1035.

Astronomy and Astrophysics

Astronomy

16

Dwarf Stars, Flare Stars, Light Curve, Stellar Spectrophotometry, Colorimetry, Energy Transfer

Scientific paper

Proxima Centauri is found to have a rate of flare production rather less than stars of similar luminosity, but very much greater than stars of similar age and higher luminosity, supporting the supposition that very low luminosity red dwarfs flare irrespective of age. The observations appear to be consistent with a two-component flare model which has hydrogen recombination as the main component.

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