The density gradient in the atmosphere of the K-type component of 31 Cygni

Dilhan EZER

doi:https://doi.org/10.1501/Commua1_0000000102

Makale detayları

The density gradient in the atmosphere of the K-type component of 31 Cygni

Yazarlar:

Dilhan EZER

Yayıncı:

Ankara University

Ana Başlıklar:

Matematik

Dergi:

Communications Faculty of Sciences University of Ankara Series A1 Mathematics and Statistics 1961 Vol.11, pp.40-60

Belge Tipi:

Makale

Yayın Tarihi:

12/1960

Belge Dili:

İngilizce

Document ID (Org No.):

2000910793

Sıklık:

Üç Aylık

eISSN:

2618-6470

pISSN:

1303-5991

DOI:

https://doi.org/10.1501/Commua1_0000000102

Özet:

 

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.

Makale detayları

The density gradient in the atmosphere of the K-type component of 31 Cygni

Yazarlar: Dilhan EZER

Yayıncı: Ankara University

Ana Başlıklar: Matematik

Dergi: Communications Faculty of Sciences University of Ankara Series A1 Mathematics and Statistics 1961 Vol.11, pp.40-60

Belge Tipi: Makale

Yayın Tarihi: 12/1960

Belge Dili: İngilizce

Document ID (Org No.): 2000910793

Sıklık: Üç Aylık

eISSN: 2618-6470

pISSN: 1303-5991

DOI: https://doi.org/10.1501/Commua1_0000000102

Sayı

Yazarlar:

Dilhan EZER

Yayıncı:

Ankara University

Ana Başlıklar:

Matematik

Dergi:

Communications Faculty of Sciences University of Ankara Series A1 Mathematics and Statistics 1961 Vol.11, pp.40-60

Belge Tipi:

Makale

Yayın Tarihi:

12/1960

Belge Dili:

İngilizce

Document ID (Org No.):

2000910793

Sıklık:

Üç Aylık

eISSN:

2618-6470

pISSN:

1303-5991

DOI:

https://doi.org/10.1501/Commua1_0000000102