Mathematical model for the 0.5 billion years aged Sun
An algorithm is given for constructing evolutionary tracks for a star with the mass equal to one solar mass. The presented model can be applied to the stars belonging to the inferior main sequence, which have the proton-proton reaction as energy source and present a radiative core and a convective s...
Gorde:
| Egile nagusia: | |
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| Formatua: | Artigo |
| Hizkuntza: | Inglês |
| Argitaratua: |
Astronomical Observatory, Department of Astronomy, Belgrade
2000-01-01
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| Saila: | Serbian Astronomical Journal |
| Sarrera elektronikoa: | http://www.doiserbia.nb.rs/img/doi/1450-698X/2000/1450-698X0062035T.pdf |
| Etiketak: |
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