Abstract
We present results of one of our ongoing projects to study the relation between radio and X-ray emission from coronal stars, viz. a survey of dM/dMe stars obtained simultaneously with ROSAT and the VLA. We find that the X-ray and radio luminosities are tightly correlated over three orders of magnitude, irrespective of spectral type. The dependence is consistent with proportionality (L R ∝ L X ).
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