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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
https://doi.org/10.1501/Commua1_0000000102
https://izlik.org/JA72DD56BK

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.

References

  • Ankara Üniversitesi Communications, Series A1:Mathematics and Statistics

Year 1961, Volume: 11 , 40 - 60, 01.01.1961
https://doi.org/10.1501/Commua1_0000000102
https://izlik.org/JA72DD56BK

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 Article
Authors

Dilhan Ezer This is me

Submission Date January 1, 1961
Publication Date January 1, 1961
DOI https://doi.org/10.1501/Commua1_0000000102
IZ https://izlik.org/JA72DD56BK
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 1.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. doi:10.1501/Commua1_0000000102
Chicago Ezer, Dilhan. 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 (January): 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 [1]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, Jan. 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 1, 1961): 40-60. https://doi.org/10.1501/Commua1_0000000102.
JAMA 1.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, Jan. 1961, pp. 40-60, doi:10.1501/Commua1_0000000102.
Vancouver 1.Dilhan Ezer. The density gradient in the atmosphere of the K-type component of 31 Cygni. Commun. Fac. Sci. Univ. Ank. Ser. A1 Math. Stat. 1961 Jan. 1;11:40-6. doi:10.1501/Commua1_0000000102

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

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