Correlation between bolometric and X-ray luminosities in RS CVn-type binaries

Details Correlation between bolometric and X-ray luminosities in RS CVn-type binaries Correlation between bolometric and X-ray luminosities in RS CVn-type binaries

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.137..195d&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 137, no. 1, Oct. 1987, p. 195-199.

Astronomy and Astrophysics

Astrophysics

2

Binary Stars, Late Stars, Stellar Activity, Stellar Luminosity, X Ray Spectra, Bolometers, Correlation, Early Stars, Stellar Coronas, Stellar Mass, Stellar Radiation

Scientific paper

Re-analysis of the X-ray emission from RS CVn-type binaries has revealed
that - contrary to the claims by many authors - their coronal activity
is not independent of bolometric luminosity (and thus mass). It becomes
clear that activity in late-type stars is also powered - just as in the
case of early-type stars - mostly by photospheric radiation.

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