No CrossRef data available.
Article contents
Chromospheric Emission and Rotation of Main Sequence Stars
Published online by Cambridge University Press: 12 April 2016
Extract
Here we present a quatitative approach to the problem of the chromospheric emission and rotation in main sequence stars based on a consistent analysis of recent published data of stars from F8 to K5. This analysis has been performed using the following physical parameters:
a) total power emission in the Call K line, Lk;
b) stellar rotation period, Prot, from chromospheric emission variability;
c) stellar ages from lithium abundance.
- Type
- Session I: General Characteristics of Active Dwarfs
- Information
- International Astronomical Union Colloquium , Volume 71: Activity in Red-Dwarf Stars , 1983 , pp. 71 - 73
- Copyright
- Copyright © Reidel 1983