Time-resolved spectroscopy and doppler tomography of UX UMa

dc.contributor.author	Suleimanov V.
dc.contributor.author	Neustroev V.
dc.contributor.author	Borisov N.
dc.contributor.author	Fioktistova I.
dc.date.accessioned	2018-09-17T21:32:36Z
dc.date.available	2018-09-17T21:32:36Z
dc.date.issued	2004
dc.identifier.issn	1405-2059
dc.identifier.uri	https://dspace.kpfu.ru/xmlui/handle/net/135128
dc.description.abstract	Medium resolution spectroscopy of nova-like cataclysmic variable UX UMA was performed using the 6-m telescope SAO RAS in April 1999. Obtained spectra cover the total orbital period including eclipse phases and allow us to reproduce the radial velocity curve. The radial-velocity variations of the Hβ emission line are found to have semi-amplitude of about 100 km/s. © Copyright 2004: IA, UNAM.
dc.relation.ispartofseries	Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias
dc.title	Time-resolved spectroscopy and doppler tomography of UX UMa
dc.type	Conference Paper
dc.relation.ispartofseries-volume	20
dc.collection	Публикации сотрудников КФУ
dc.relation.startpage	270
dc.source.id	SCOPUS14052059-2004-20-SID33846018746

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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.