Coronal densities from X-ray rotational modulation.

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Stellar Coronae: X Rays, Stellar Coronae: Electron Densities, Stellar Coronae: Stellar Rotation

Scientific paper

The authors present a geometric method for estimating lower limits of
coronal densities based on X-ray rotational modulation of single stars.
Application to two young, very active solar-like stars yields electron
densities of several times 1010cm-3 or more.

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