CaII and MgII excess flux density in cool stars (Rutten, 1987)

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Scientific paper

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Stars: Late-Type, Stars: Dwarfs, Stars: Giant, Magnitudes: Absolute

Scientific paper

The relation between the CaII H and K line-tore flux density and rotation period is studied for a sample of 313 cool stars of luminosity classes ranging from II-III to V, and compared to similar relations for MgII h and k and soft X-ray.
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