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    RS CVn binaries: Testing the solar-stellar dynamo connection (1995)
    In:  CASI
    Details
    Publication Date: 2019-06-28
    Description: We have used the Extreme Ultraviolet Explorer satellite to study the coronal emission from the EUV-bright RS CVn binaries Sigma2 CrB, observed February 10-21, 1994, and II Peg, observed October 1-5, 1993. We present time-resolved and integrated EUV short-, medium-, and long-wavelength spectra for these binaries. Sigma2 CrB shows significant first-order emission features in the long-wavelength region. The coronal emission distributions and electron densities are estimated for those active coronae dominated by high temperature plasma.
    Keywords: ASTRONOMY
    Type: NASA-CR-199872 , NAS 1.26:199872 , NIPS-96-08161
    Format: application/pdf
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