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

Year 1961, Volume: 11 , 40 - 60, 01.01.1961

Dilhan Ezer

https://doi.org/10.1501/Commua1_0000000102

Abstract

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

References

  • Ankara Üniversitesi Communications, Series A1:Mathematics and Statistics

Year 1961, Volume: 11 , 40 - 60, 01.01.1961

Dilhan Ezer

https://doi.org/10.1501/Commua1_0000000102

Abstract

References

  • Ankara Üniversitesi Communications, Series A1:Mathematics and Statistics
There are 1 citations in total.

Details

Primary Language English
Subjects Mathematical Sciences
Journal Section Research Articles
Authors

Dilhan Ezer This is me

Publication Date January 1, 1961
Submission Date January 1, 1961
Published in Issue Year 1961 Volume: 11

Cite

APA Ezer, D. (1961). The density gradient in the atmosphere of the K-type component of 31 Cygni. Communications Faculty of Sciences University of Ankara Series A1 Mathematics and Statistics, 11, 40-60. https://doi.org/10.1501/Commua1_0000000102
AMA Ezer D. The density gradient in the atmosphere of the K-type component of 31 Cygni. Commun. Fac. Sci. Univ. Ank. Ser. A1 Math. Stat. January 1961;11:40-60. doi:10.1501/Commua1_0000000102
Chicago Ezer, Dilhan. “The Density Gradient in the Atmosphere of the K-Type Component of 31 Cygni”. Communications Faculty of Sciences University of Ankara Series A1 Mathematics and Statistics 11, January (January 1961): 40-60. https://doi.org/10.1501/Commua1_0000000102.
EndNote Ezer D (January 1, 1961) The density gradient in the atmosphere of the K-type component of 31 Cygni. Communications Faculty of Sciences University of Ankara Series A1 Mathematics and Statistics 11 40–60.
IEEE D. Ezer, “The density gradient in the atmosphere of the K-type component of 31 Cygni”, Commun. Fac. Sci. Univ. Ank. Ser. A1 Math. Stat., vol. 11, pp. 40–60, 1961, doi: 10.1501/Commua1_0000000102.
ISNAD Ezer, Dilhan. “The Density Gradient in the Atmosphere of the K-Type Component of 31 Cygni”. Communications Faculty of Sciences University of Ankara Series A1 Mathematics and Statistics 11 (January 1961), 40-60. https://doi.org/10.1501/Commua1_0000000102.
JAMA Ezer D. The density gradient in the atmosphere of the K-type component of 31 Cygni. Commun. Fac. Sci. Univ. Ank. Ser. A1 Math. Stat. 1961;11:40–60.
MLA Ezer, Dilhan. “The Density Gradient in the Atmosphere of the K-Type Component of 31 Cygni”. Communications Faculty of Sciences University of Ankara Series A1 Mathematics and Statistics, vol. 11, 1961, pp. 40-60, doi:10.1501/Commua1_0000000102.
Vancouver Ezer D. The density gradient in the atmosphere of the K-type component of 31 Cygni. Commun. Fac. Sci. Univ. Ank. Ser. A1 Math. Stat. 1961;11:40-6.

Communications Faculty of Sciences University of Ankara Series A1 Mathematics and Statistics.

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