Two-component theoretical chromosphere models for K dwarfs of different magnetic activity: exploring the Ca II emission-stellar rotation relationship
Gespeichert in:
| Hauptverfasser: | , , , , |
|---|---|
| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
1999
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| In: |
The astrophysical journal
Year: 1999, Jahrgang: 522, Heft: 2, Pages: 1053-1068 |
| ISSN: | 1538-4357 |
| DOI: | 10.1086/307689 |
| Online-Zugang: | Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1086/307689 Verlag, kostenfrei, Volltext: http://iopscience.iop.org/article/10.1086/307689/meta 
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| Verfasserangaben: | M. Cuntz, W. Rammacher, P. Ulmschneider, Z.E. Musielak and S.H. Saar |
MARC
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