| Autor: |
Gürkan Aslan, Ian Steer, Faruk Soydugan, Mehmet Alpsoy, F. Alicavus, Esin Soydugan, Volkan Bakiş, Selçuk Bilir, Hicran Bakiş, Zeki Eker |
| Rok vydání: |
2018 |
| Předmět: |
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| Popis: |
Conventional mass-luminosity (M – L) relations are defined using 509 nearby main-sequence (MS) stars within the Solar neighborhood. A smooth mass-radius (M – R) relation was fixed from radii of MS stars appeared in literature having masses within the limits 0.179 – 1.5 M⊙. Similarly, a smooth mass-effective temperature (M – Teff) relation was derived for the main-sequence stars having masses within the limits 1.5 – 31 M⊙ using their effective temperatures available. The omitted parts of M – R and M – Teff relations in the range from 0.179 to 31 M⊙ were computed according to Stephan-Boltzmann law, so inter-related M – L, M – R and M – Teff were achieved.Conventional mass-luminosity (M – L) relations are defined using 509 nearby main-sequence (MS) stars within the Solar neighborhood. A smooth mass-radius (M – R) relation was fixed from radii of MS stars appeared in literature having masses within the limits 0.179 – 1.5 M⊙. Similarly, a smooth mass-effective temperature (M – Teff) relation was derived for the main-sequence stars having masses within the limits 1.5 – 31 M⊙ using their effective temperatures available. The omitted parts of M – R and M – Teff relations in the range from 0.179 to 31 M⊙ were computed according to Stephan-Boltzmann law, so inter-related M – L, M – R and M – Teff were achieved. |
| Databáze: |
OpenAIRE |
| Externí odkaz: |
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