EUVE Coronal Spectroscopy of the RS CVn Binaries sigma (2) CrB and II Peg

Details EUVE Coronal Spectroscopy of the RS CVn Binaries sigma (2) CrB and II Peg EUVE Coronal Spectroscopy of the RS CVn Binaries sigma (2) CrB and II Peg

May 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994aas...184.0517b&link_type=abstract

American Astronomical Society, 184th AAS Meeting, #05.17; Bulletin of the American Astronomical Society, Vol. 26, p.865

Astronomy and Astrophysics

Astronomy

Scientific paper

We have used the Extreme Ultraviolet Explorer satellite to study the coronal emission from the EUV-bright RS CVn binaries sigma (2) CrB, observed 1994 Feb 16-21, and II Peg, observed 1993 Oct 1-5. We present time-resolved and integrated EUV short, medium and long wavelength spectra for these binaries. sigma (2) CrB shows significant first-order emission features in the long wavelength region. The coronal emission measure distributions and electron densities are estimated for these active coronae dominated by high temperature (>= 10(7) K) plasma. This work is supported by NASA Grants NAG5-2259 & NAGW-2904 to the University of Colorado.

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