ISSN: 2310-757X
Пожалуйста, используйте этот идентификатор, чтобы цитировать или ссылаться на этот ресурс:
http://elar.urfu.ru/handle/10995/101772Полная запись метаданных
| Поле DC | Значение | Язык |
|---|---|---|
| dc.contributor.author | Staritsin, E. I. | en |
| dc.date.accessioned | 2021-08-31T14:59:38Z | - |
| dc.date.available | 2021-08-31T14:59:38Z | - |
| dc.date.issued | 2019 | - |
| dc.identifier.citation | Staritsin E. I. Is the additional increase of star luminosity due to partial mixing real? / E. I. Staritsin. — DOI 10.1088/1674-4527/19/3/32 // Research in Astronomy and Astrophysics. — 2019. — Vol. 19. — Iss. 3. — 032. | en |
| dc.identifier.issn | 16744527 | - |
| dc.identifier.other | Final | 2 |
| dc.identifier.other | All Open Access, Green | 3 |
| dc.identifier.other | https://www.scopus.com/inward/record.uri?eid=2-s2.0-85065055626&doi=10.1088%2f1674-4527%2f19%2f3%2f32&partnerID=40&md5=bac0dd9757bb85e0095ae06e118193d0 | |
| dc.identifier.other | http://arxiv.org/pdf/1805.12412 | m |
| dc.identifier.uri | http://elar.urfu.ru/handle/10995/101772 | - |
| dc.description.abstract | The partial mixing of matter between the radiative envelope and convective core in an early B-type star produces an additional increase of star luminosity during main sequence evolution. High quality data on stellar mass and luminosity defined from studies of detached double-lined eclipsing binaries are used to check the existence of such additional increase. It is shown that the additional luminosity increase does not contradict observed high quality data, if the intensity of partial mixing is restricted by the observed increase in surface helium content. © 2019 National Astronomical Observatories, CAS and IOP Publishing Ltd.. | en |
| dc.format.mimetype | application/pdf | en |
| dc.language.iso | en | en |
| dc.publisher | Institute of Physics Publishing | en |
| dc.rights | info:eu-repo/semantics/openAccess | en |
| dc.source | Res. Astron. Astrophys. | 2 |
| dc.source | Research in Astronomy and Astrophysics | en |
| dc.subject | STARS: STRUCTURE AND EVOLUTION | en |
| dc.title | Is the additional increase of star luminosity due to partial mixing real? | en |
| dc.type | Article | en |
| dc.type | info:eu-repo/semantics/article | en |
| dc.type | info:eu-repo/semantics/publishedVersion | en |
| dc.identifier.doi | 10.1088/1674-4527/19/3/32 | - |
| dc.identifier.scopus | 85065055626 | - |
| local.contributor.employee | Staritsin, E.I., K. A. Barkhatova Kourovka Astronomical Observatory, B.N. Yeltsin Ural Federal University, pr. Lenina 51, Ekaterinburg, 620000, Russian Federation | |
| local.issue | 3 | - |
| local.volume | 19 | - |
| dc.identifier.wos | 000462485200002 | - |
| local.contributor.department | K. A. Barkhatova Kourovka Astronomical Observatory, B.N. Yeltsin Ural Federal University, pr. Lenina 51, Ekaterinburg, 620000, Russian Federation | |
| local.identifier.pure | 9188936 | - |
| local.description.order | 032 | - |
| local.identifier.eid | 2-s2.0-85065055626 | - |
| local.identifier.wos | WOS:000462485200002 | - |
| Располагается в коллекциях: | Научные публикации ученых УрФУ, проиндексированные в SCOPUS и WoS CC | |
Файлы этого ресурса:
| Файл | Описание | Размер | Формат | |
|---|---|---|---|---|
| 2-s2.0-85065055626.pdf | 162,46 kB | Adobe PDF | Просмотреть/Открыть |
Все ресурсы в архиве электронных ресурсов защищены авторским правом, все права сохранены.