Is WD 1437-008 a cataclysmic variable?

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]
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