Two-component theoretical chromosphere models for K dwarfs of different magnetic activity: Exploring the Ca II emission-stellar rotation relationship

Astrophysical Journal

Volumn 522, Issue 2 PART 1, 1999, Pages 1053-1068

  Cuntz, M ^a   Rammacher, W ^b   Ulmschneider, P ^b   Musielak, Z E ^a,b,c   Saar, S H ^d  

^a UNIVERSITY OF ALABAMA IN HUNTSVILLE   (United States)

^b UNIVERSITY OF HEIDELBERG   (Germany)

^c UNIVERSITY OF TEXAS AT ARLINGTON   (United States)

^d HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

Author keywords

Line: formation; MHD; Stars: activity; Stars: chromospheres; Stars: late type; Stars: rotation

Indexed keywords

EID: 0033543367     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/307689     Document Type: Article

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