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Is WD 1437-008 a cataclysmic variable?
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| dc.contributor.author | Shimansky V. | |
| dc.contributor.author | Nurtdinova D. | |
| dc.contributor.author | Borisov N. | |
| dc.contributor.author | Spiridonova O. | |
| dc.date.accessioned | 2018-09-18T20:30:55Z | |
| dc.date.available | 2018-09-18T20:30:55Z | |
| dc.date.issued | 2011 | |
| dc.identifier.issn | 1990-3413 | |
| dc.identifier.uri | https://dspace.kpfu.ru/xmlui/handle/net/140669 | |
| dc.description.abstract | Comprehensive observations of a close binary candidate WD 1437-008 are performed. The shape and amplitude of the observed brightness variations are shown to be inconsistent with the hypothesis of reflection effects, and the photometric period of the system, P phot = 0. d2775, is found to differ from the period of spectral variations, P sp = 0. d272060. As a result, WD 1437-008 has been preliminarily classified as a low-inclination cataclysmic variable. © 2011 Pleiades Publishing, Ltd. | |
| dc.relation.ispartofseries | Astrophysical Bulletin | |
| dc.subject | stars: dwarf novae | |
| dc.subject | stars: individual: WD 1437-008 | |
| dc.subject | stars: variables: general | |
| dc.title | Is WD 1437-008 a cataclysmic variable? | |
| dc.type | Article | |
| dc.relation.ispartofseries-issue | 4 | |
| dc.relation.ispartofseries-volume | 66 | |
| dc.collection | Публикации сотрудников КФУ | |
| dc.relation.startpage | 442 | |
| dc.source.id | SCOPUS19903413-2011-66-4-SID82055193414 |
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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.