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

Dilhan Ezer

doi:10.1501/Commua1_0000000102

EN

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

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

References

Ankara Üniversitesi Communications, Series A1:Mathematics and Statistics

Details

Primary Language

English

Subjects

Mathematical Sciences

Journal Section

Research Article

Authors

Dilhan Ezer This is me
Türkiye

Publication Date

January 1, 1961

Submission Date

January 1, 1961

Acceptance Date

-

Published in Issue

Year 1961 Volume: 11

DOI

https://doi.org/10.1501/Commua1_0000000102

IZ

https://izlik.org/JA72DD56BK

Cite

RIS / Bibtex

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