EXOSAT observations of late-type stars - The application of coronal loop models

Details EXOSAT observations of late-type stars - The application of coronal loop models EXOSAT observations of late-type stars - The application of coronal loop models

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ssrv...40...43l&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

4

Coronal Loops, Exosat Satellite, Late Stars, Stellar Models, Ultraviolet Spectra, X Ray Spectra, Iue, Spaceborne Astronomy, Spectral Energy Distribution, Stellar Temperature

Scientific paper

The application of solar-type coronal loop models to X-ray and ultraviolet observations of late-type stars is discussed. The observations were carried out using the Channel Multiplier Array (CMA) and Low Energy telescope (LE 1) on board Exosat, together with the Imaging Proportional Counter (IPC) instrument on board the Einstein Observatory. Constraints are derived for the temperature, pressure, and size of the emitting structures in selected F8 and G5 stars together with some BY Dra variables. The predicted surface flux at earth is given as a function of wavelength over the spectral range 1-2000 for the outer atmosphere of K Ceti.

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