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Colors and patterns of black hole X-ray binary GX 339-4

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dc.contributor.author Kosenkov I.A.
dc.contributor.author Veledina A.
dc.contributor.author Suleimanov V.F.
dc.contributor.author Poutanen J.
dc.date.accessioned 2021-02-24T20:31:39Z
dc.date.available 2021-02-24T20:31:39Z
dc.date.issued 2020
dc.identifier.issn 0004-6361
dc.identifier.uri https://dspace.kpfu.ru/xmlui/handle/net/160715
dc.description.abstract © ESO 2020. Black hole X-ray binaries show signs of nonthermal emission in the optical to near-infrared range. We analyzed optical to near-infrared SMARTS data on GX 339-4 over the 2002-2011 period. Using soft state data, we estimated the interstellar extinction toward the source and characteristic color temperatures of the accretion disk. We show that various spectral states of regular outbursts occupy similar regions on color-magnitude diagrams, and that transitions between the states proceed along the same tracks despite substantial differences in the morphology of the observed light curves. We determine the typical duration of hard-to-soft and soft-to-hard state transitions and the hard state at the decaying stage of the outburst to be one, two, and four weeks, respectively. We find that the failed outbursts cannot be easily distinguished from the regular outbursts at their early stages, but if the source reaches 16 mag in V band, it transits to the soft state. By subtracting the contribution of the accretion disk, we obtain spectra of the nonthermal component, which have constant, nearly flat shapes during the transitions between the hard and soft states. In contrast to the slowly evolving nonthermal component seen at optical and near-infrared wavelengths, the mid-infrared spectrum is strongly variable on short timescales and sometimes shows a prominent excess with a cutoff below 1014 Hz. We show that the radio to optical spectrum can be modeled using three components corresponding to the jet, hot flow, and irradiated accretion disk.
dc.relation.ispartofseries Astronomy and Astrophysics
dc.subject Accretion, accretion disks
dc.subject Black hole physics
dc.subject Methods: data analysis
dc.subject Stars: black holes
dc.subject Stars: individual: GX 339-4
dc.subject X-rays: binaries
dc.title Colors and patterns of black hole X-ray binary GX 339-4
dc.type Article
dc.relation.ispartofseries-volume 638
dc.collection Публикации сотрудников КФУ
dc.source.id SCOPUS00046361-2020-638-SID85088252643


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  • Публикации сотрудников КФУ Scopus [22633]
    Коллекция содержит публикации сотрудников Казанского федерального (до 2010 года Казанского государственного) университета, проиндексированные в БД Scopus, начиная с 1970г.

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