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.
Roentgenstrahlung from the Universe
- Pub Date:
- February 1996
- Stellar Coronae: X Rays;
- Stellar Coronae: Electron Densities;
- Stellar Coronae: Stellar Rotation