Research Article

Stellar Mass-Radius Relation

Volume: 38 January 1, 1989
  • Osman Demircan
Communications Faculty of Sciences University of Ankara Series A2-A3 Physical Sciences and Engineering Cover
Communications Faculty of Sciences University of Ankara Series A2-A3 Physical Sciences and Engineering
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Stellar Mass-Radius Relation

Abstract

The stellar mass-radius relation is determined by using new data on absolute dimensions of the components of well-detached binary systems. The relation is compared with the published empirical and theoretical mass-radins relations. The location of the knee in the empirical relation is estimated in 1.66 solar mass. The results can be useful (i) in estimating the masses of MS stars vvhich are not components of binary systems.

Keywords

References

  1. Ankara Üniversitesi- Ankara Üniversitesi Communications, Series A2-A3: Physical Sciences and Enginering Dergisi

Details

Primary Language

English

Subjects

Engineering

Journal Section

Research Article

Authors

Osman Demircan This is me
Türkiye

Publication Date

January 1, 1989

Submission Date

January 1, 1989

Acceptance Date

-

Published in Issue

Year 1989 Volume: 38

DOI

https://doi.org/10.1501/commua1-2_0000000057

IZ

https://izlik.org/JA48XY85WM

Cite

RIS / Bibtex
APA
Demircan, O. (1989). Stellar Mass-Radius Relation. Communications Faculty of Sciences University of Ankara Series A2-A3 Physical Sciences and Engineering, 38, 9-16. https://doi.org/10.1501/commua1-2_0000000057
AMA
1.Demircan O. Stellar Mass-Radius Relation. Commun.Fac.Sci.Univ.Ank.Series A2-A3: Phys.Sci. and Eng. 1989;38:9-16. doi:10.1501/commua1-2_0000000057
Chicago
Demircan, Osman. 1989. “Stellar Mass-Radius Relation”. Communications Faculty of Sciences University of Ankara Series A2-A3 Physical Sciences and Engineering 38 (January): 9-16. https://doi.org/10.1501/commua1-2_0000000057.
EndNote
Demircan O (January 1, 1989) Stellar Mass-Radius Relation. Communications Faculty of Sciences University of Ankara Series A2-A3 Physical Sciences and Engineering 38 9–16.
IEEE
[1]O. Demircan, “Stellar Mass-Radius Relation”, Commun.Fac.Sci.Univ.Ank.Series A2-A3: Phys.Sci. and Eng., vol. 38, pp. 9–16, Jan. 1989, doi: 10.1501/commua1-2_0000000057.
ISNAD
Demircan, Osman. “Stellar Mass-Radius Relation”. Communications Faculty of Sciences University of Ankara Series A2-A3 Physical Sciences and Engineering 38 (January 1, 1989): 9-16. https://doi.org/10.1501/commua1-2_0000000057.
JAMA
1.Demircan O. Stellar Mass-Radius Relation. Commun.Fac.Sci.Univ.Ank.Series A2-A3: Phys.Sci. and Eng. 1989;38:9–16.
MLA
Demircan, Osman. “Stellar Mass-Radius Relation”. Communications Faculty of Sciences University of Ankara Series A2-A3 Physical Sciences and Engineering, vol. 38, Jan. 1989, pp. 9-16, doi:10.1501/commua1-2_0000000057.
Vancouver
1.Osman Demircan. Stellar Mass-Radius Relation. Commun.Fac.Sci.Univ.Ank.Series A2-A3: Phys.Sci. and Eng. 1989 Jan. 1;38:9-16. doi:10.1501/commua1-2_0000000057

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