Minimum level of X-ray emission in solar-type stars

Details Minimum level of X-ray emission in solar-type stars Minimum level of X-ray emission in solar-type stars

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990azh....67.1261t&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 67, Nov.-Dec. 1990, p. 1261-1270. In Russian.

Astronomy and Astrophysics

Astronomy

F Stars, G Stars, K Stars, Stellar Radiation, X Ray Stars, Chromosphere, Emission Spectra, Stellar Activity, Stellar Coronas, Stellar Spectra

Scientific paper

A base curve for X-ray emission flux density FX(B-V) is determined by
comparing chromospheric and coronal activity indices of 50 main-sequence
F-K-type stars. The form of this curve does not contradict the
hypothesis of the same coronal-heating mechanism for quiet and active
stars.

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