| Autor: |
O. P. Paramonova, T. V. Mishenina, O. Chepizhko |
| Jazyk: |
angličtina |
| Rok vydání: |
2013 |
| Předmět: |
|
| Zdroj: |
Odessa Astronomical Publications, Vol 26, Iss 1 (2013) |
| Druh dokumentu: |
article |
| ISSN: |
1810-4215 |
| DOI: |
10.18524/1810-4215.2013.26.82199 |
| Popis: |
The sulfur abundance was determined by the synthetic spectrum method in the stars with metallicity close to that of the Sun. The comparison with the results of other authors, as well as the nucleosynthesis computations were made. |
| Databáze: |
Directory of Open Access Journals |
| Externí odkaz: |
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