X-ray Emission from Single Stars

Details X-ray Emission from Single Stars X-ray Emission from Single Stars

Jan 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004iaus..219..187s&link_type=abstract

Stars as suns : activity, evolution and planets, Proceedings of the 219th symposium of the International Astronomical Union held

Astronomy and Astrophysics

Astronomy

Scientific paper

I will present the results of extensive surveys for X-ray emission from solar-like stars in the solar vicinity. The main results of these studies are: (a) All stars main sequence stars with outer convection zones are surrounded by hot coronae; (b) There exists a minimal X-ray surface flux similar to the surface flux from coronal holes; (c) Large variations in X-ray flux are uncommon at least for stars of spectral type earlier than M. The X-ray properties of stars will be compared to those of the Sun and it will be explored to what extent the magnetic activity paradigm holds for stars of type A and earlier and for stars below the MS cut off.

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