EXOSAT observations of M dwarfs

Details EXOSAT observations of M dwarfs EXOSAT observations of M dwarfs

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ssrv...40...69s&link_type=abstract

(ESA, ESLAB Symposium on X-Ray Astronomy in the EXOSAT Era, 18th, The Hague, Netherlands, Nov. 5-9, 1984) Space Science Reviews

Astronomy and Astrophysics

Astronomy

5

Dwarf Stars, Exosat Satellite, M Stars, Stellar Coronas, Stellar Spectrophotometry, Coronal Loops, Emission Spectra, Spaceborne Astronomy, Stellar Temperature, X Ray Sources

Scientific paper

The authors give a progress report of their EXOSAT observations of active M dwarfs. The possibilities of filter spectroscopy of coronal X-ray sources using the available CMA filters are discussed, and the authors confirm that M dwarfs are rather hot coronal sources with X-ray temperatures in excess of 107K, a result previously obtained with the Einstein Observatory.

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