Coronae on stars

Details Coronae on stars Coronae on stars

Mar 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986iraj...17..200h&link_type=abstract

Irish Astronomical Journal (ISSN 0021-1052), vol. 17, March 1986, p. 200-216. Research supported by the Lockheed Independent Res

Astronomy and Astrophysics

Astronomy

10

Solar Corona, Stellar Coronas, Coronal Loops, Dwarf Stars, Early Stars, Hertzsprung-Russell Diagram, Late Stars, M Stars, Main Sequence Stars, Stellar Flares

Scientific paper

Three lines of evidence are noted to point to a flare heating source for stellar coronae: a strong correlation between time-averaged flare energy release and coronal X-ray luminosity, the high temperature flare-like component of the spectral signature of coronal X-ray emission, and the observed short time scale variability that indicates continuous flare activity. It is presently suggested that flares may represent only the extreme high energy tail of a continuous distribution of coronal energy release events.

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