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dc.contributor.author Drozd, K.
dc.contributor.author Swierczynski, E.
dc.contributor.author Ragan, E.
dc.date.accessioned 2017-06-04T18:58:02Z
dc.date.available 2017-06-04T18:58:02Z
dc.date.issued 2012
dc.identifier.citation V407 Cygni - nova like outburst in symbiotic system / K. Drozd, E. Swierczynski, E. Ragan // Advances in Astronomy and Space Physics. — 2012. — Т. 2., вип. 2. — С. 132-134. — Бібліогр.: 16 назв. — англ. uk_UA
dc.identifier.issn 2227-1481
dc.identifier.uri http://dspace.nbuv.gov.ua/handle/123456789/119182
dc.description.abstract We presented spectroscopic and photometric observations of V407 Cygni obtained during 2006-2011. Our data shows the different activity stages connected with the two components of this symbiotic binary system. Cool giant exhibits pulsation character typical for Mira-type stars. Simultaneously, classical nova outburst connected with hot white dwarf was observed in 2010. Multicolour photometry and spectra obtained in a wide wave range are necessary to understand behaviour of such extreme binary. Our long-term observations together with gamma-ray, X-ray and radio monitoring reported by other authors covered the whole spectral domain and provide a lot of useful information about the nature of V407 Cyg. uk_UA
dc.description.sponsorship We are thankful to former students of Nicolaus Copernicus University, Cezary Galan and Piotr Wychudzki for making part of the photometric observations. This work was partially supported by Nicolaus Copernicus University grant no. 416-A. uk_UA
dc.language.iso en uk_UA
dc.publisher Головна астрономічна обсерваторія НАН України uk_UA
dc.relation.ispartof Advances in Astronomy and Space Physics
dc.title V407 Cygni - nova like outburst in symbiotic system uk_UA
dc.type Article uk_UA
dc.status published earlier uk_UA

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