The density gradient in the atmosphere of the K-type component of 31 Cygni
The density gradient in the atmosphere of the K-type component of 31 Cygni
The discovery of turbulent motions in the atmosphere of supergiant stars, made it increasingly important to study the structure of such atmospheres. The best clues to the structure of supergiant atmospheres come from the studies of eclipsing Systems.
Keywords:
The density, Atmosphere of the K-type Component of 31 Cygi,
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- Ankara Üniversitesi Communications, Series A1:Mathematics and Statistics
- ISSN: 1303-5991
- Yayın Aralığı: Yılda 4 Sayı
- Başlangıç: 1948
- Yayıncı: Ankara Üniversitesi