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...
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| Hlavní autor: | |
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| Médium: | Artigo |
| Jazyk: | Inglês |
| Vydáno: |
Astronomical Observatory, Department of Astronomy, Belgrade
2000-01-01
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| Edice: | Serbian Astronomical Journal |
| On-line přístup: | http://www.doiserbia.nb.rs/img/doi/1450-698X/2000/1450-698X0062035T.pdf |
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