Stellar Activity–Phenomenology and General Principles
Author:
Publisher
Springer International Publishing
Link
http://link.springer.com/content/pdf/10.1007/978-3-030-11452-7_2
Reference27 articles.
1. Buchholz, B., Ulmschneider, P., Cuntz, M.: Basal heating in main-sequence stars and giants: results from monochromatic acoustic wave models. Astrophys. J. 494, 700 (1998)
2. Cardini, D.: Mg II chromospheric radiative loss rates in cool active and quiet stars. Astron. Astrophys. 430, 303 (2005)
3. Carlsson, M., Stein, R.F.: Does a nonmagnetic solar chromosphere exist? Astrophys. J. Lett. 440, L29 (1995)
4. Cranmer, S.R., Saar, S.H.: Testing a predictive theoretical model for the mass-loss rates of cool stars. Astrophys. J. 741, 23 (2011)
5. Cuntz, M., Rammacher, W., Ulmschneider, P., Musielak, Z.E., Saar, S.H.: Two-component theoretical chromosphere models for K dwarfs of different magnetic activity: exploring the Ca II emission-stellar rotation relationship. Astrophys. J. 522, 1053 (1999)
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