Sulfur abundance in the Galactic disc stars
| dc.contributor.author | Paramonova, Olga P. | en |
| dc.contributor.author | Mishenina, Tamara V. | en |
| dc.contributor.author | Chepizhko, Oleksandr O. | en |
| dc.contributor.author | Парамонова, Ольга Петрівна | uk |
| dc.contributor.author | Мішеніна, Тамара Василівна | uk |
| dc.contributor.author | Чепіжко, Олександр Олександрович | uk |
| dc.date.accessioned | 2014-03-28T07:43:49Z | |
| dc.date.available | 2014-03-28T07:43:49Z | |
| dc.date.issued | 2013 | |
| dc.description.abstract | 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. | en |
| dc.identifier.citation | Odessa Astronomical Publications | en |
| dc.identifier.uri | https://dspace.onu.edu.ua/handle/123456789/4779 | |
| dc.language.iso | en | |
| dc.publisher | Astroprint | en |
| dc.relation.ispartofseries | ;vol. 26, issue 1, p. 94 | |
| dc.subject | stars: abundance | en |
| dc.subject | stars: late-type | en |
| dc.title | Sulfur abundance in the Galactic disc stars | en |
| dc.type | Article | en |
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