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Vega: Data analysis of the observations
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| dc.contributor.author | Merezhin V. | |
| dc.date.accessioned | 2018-09-14T20:04:57Z | |
| dc.date.available | 2018-09-14T20:04:57Z | |
| dc.date.issued | 1990 | |
| dc.identifier.issn | 0004-640X | |
| dc.identifier.uri | https://dspace.kpfu.ru/xmlui/handle/net/132104 | |
| dc.description.abstract | The observational data analysis indicates that the star is enveloped into a nebula considerably stretched along the equatorial plane. Vega is a star with B9.5IV-V characteristics with Te=10.105±230 K and R=2.69±0.25 R⊙. The cover deforms energy distribution in Vega spectrum. As a result, the energy from with distribution corresponding to an A0V star is imitated in the direction towards the observer. © 1990 Kluwer Academic Publishers. | |
| dc.relation.ispartofseries | Astrophysics and Space Science | |
| dc.title | Vega: Data analysis of the observations | |
| dc.type | Article | |
| dc.relation.ispartofseries-issue | 2 | |
| dc.relation.ispartofseries-volume | 174 | |
| dc.collection | Публикации сотрудников КФУ | |
| dc.relation.startpage | 181 | |
| dc.source.id | SCOPUS0004640X-1990-174-2-SID34249952943 |
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Публикации сотрудников КФУ Scopus [24551]
Коллекция содержит публикации сотрудников Казанского федерального (до 2010 года Казанского государственного) университета, проиндексированные в БД Scopus, начиная с 1970г.