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The mass of the black hole in the X-ray binary LMC X-1

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dc.contributor.author Abubekerov M.
dc.contributor.author Antokhina E.
dc.contributor.author Gostev N.
dc.contributor.author Cherepashchuk A.
dc.contributor.author Shimansky V.
dc.date.accessioned 2018-09-19T20:51:25Z
dc.date.available 2018-09-19T20:51:25Z
dc.date.issued 2016
dc.identifier.issn 1063-7729
dc.identifier.uri https://dspace.kpfu.ru/xmlui/handle/net/143346
dc.description.abstract © 2016, Pleiades Publishing, Ltd.A dynamical estimate of the mass of the black hole in the LMC X-1 binary system is obtained in the framework of a Roche model for the optical star, based on fitting of the He I 4471 Å and He II 4200 Å absorption lines assuming LTE. The mass of the black hole derived from the radial-velocity curve for the He II 4200 Å line is mx = 10.55 M⊙, close to the value found earlier based on a model with two point bodies [1].
dc.relation.ispartofseries Astronomy Reports
dc.title The mass of the black hole in the X-ray binary LMC X-1
dc.type Article
dc.relation.ispartofseries-issue 12
dc.relation.ispartofseries-volume 60
dc.collection Публикации сотрудников КФУ
dc.relation.startpage 1029
dc.source.id SCOPUS10637729-2016-60-12-SID84996565694


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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.

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