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.
Birincil Dil | İngilizce |
---|---|
Konular | Mühendislik |
Bölüm | Research Article |
Yazarlar | |
Yayımlanma Tarihi | 1 Ocak 1989 |
Gönderilme Tarihi | 1 Ocak 1989 |
Yayımlandığı Sayı | Yıl 1989 |
Communications Faculty of Sciences University of Ankara Series A2-A3 Physical Sciences and Engineering
This work is licensed under a Creative Commons Attribution 4.0 International License.