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Supersoft X-ray sources. Parameters of stellar atmospheres
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| dc.contributor.author | Ibragimov A. | |
| dc.contributor.author | Suleǐmanov V. | |
| dc.contributor.author | Vikhlinin A. | |
| dc.contributor.author | Sakhibullin N. | |
| dc.date.accessioned | 2018-09-17T21:10:36Z | |
| dc.date.available | 2018-09-17T21:10:36Z | |
| dc.date.issued | 2003 | |
| dc.identifier.issn | 1063-7729 | |
| dc.identifier.uri | https://dspace.kpfu.ru/xmlui/handle/net/134628 | |
| dc.description.abstract | ROSAT spectra of 11 supersoft X-ray sources are approximated with theoretical spectra obtained in LTE models for the atmospheres of hot white dwarfs with line blanketing. The confidence intervals of parameters derived from these approximations-Teff, log, g, NH, and R2/d2 - are determined. The results are compared with predictions for a model with stable/recurrent thermonuclear burning on the white-dwarf surface. © 2003 MAIK "Nauka/Interperiodica". | |
| dc.relation.ispartofseries | Astronomy Reports | |
| dc.title | Supersoft X-ray sources. Parameters of stellar atmospheres | |
| dc.type | Article | |
| dc.relation.ispartofseries-issue | 3 | |
| dc.relation.ispartofseries-volume | 47 | |
| dc.collection | Публикации сотрудников КФУ | |
| dc.relation.startpage | 186 | |
| dc.source.id | SCOPUS10637729-2003-47-3-SID0344950438 |
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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.