Chromospheric/coronal emission correlations in 'quiescent' and eruptive phenomena in M-dwarf stars

Details Chromospheric/coronal emission correlations in 'quiescent' and eruptive phenomena in M-dwarf stars Chromospheric/coronal emission correlations in 'quiescent' and eruptive phenomena in M-dwarf stars

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...240..357m&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 240, no. 2, Dec. 1990, p. 357-359. Research supported by SERC.

Astronomy and Astrophysics

Astrophysics

6

Chromosphere, Dwarf Stars, Emission Spectra, M Stars, Stellar Coronas, H Alpha Line, H Gamma Line, Stellar Flares, Stellar Spectra, X Rays

Scientific paper

A power correlation between 'quiescent' and flaring H-gamma and X-ray
emission is presented for a group of active dwarf M stars. The
relationship holds for both 'quiescent' and flaring conditions for
several orders of magnitude change in energy. Explanations in terms of
X-ray back-heating and microflaring are discussed.

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