V407 Cyg and RS Oph - comparison of two exotic variables

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dc.contributor.authorDrozd, K.
dc.contributor.authorSwierczynski, E.
dc.contributor.authorRagan, E.
dc.contributor.authorBuil, C.
dc.date.accessioned2017-06-07T18:17:29Z
dc.date.available2017-06-07T18:17:29Z
dc.date.issued2013
dc.description.abstractV407 Cygni and RS Ophiuchi are two similar but unique objects. It can be said that they each belong to an individual type of stars. During their quiet state they seem to be symbiotic stars. However, both stars have previously displayed nova-like outbursts. We would like to take a closer look at these two unique objects, and to compare them. We presented spectroscopic and photometric observations of V407 Cyg and RS Oph obtained throughout the period from 2006 until 2013. Our data show the di erent activity stages connected with the two components of these binary systems. Multicolour photometry and spectra obtained in a wide frequency range are utilized to understand the behaviour of such extremely binaries.uk_UA
dc.description.sponsorshipWe are greatful to former students of Nicolaus Copernicus University, Cezary Galan and Piotr Wychudzki, for conducting part of the photometric observations, and Agnieszka Fidos, Jedrzej Osiwala, Grzegorz Rycyk, and Malgorzata Wozniak, for conducting part of the spectroscopic observations.uk_UA
dc.identifier.citationV407 Cyg and RS Oph - comparison of two exotic variables / K. Drozd, E. Swierczynski, E. Ragan, C. Buil // Advances in Astronomy and Space Physics. — 2013. — Т. 3., вип. 2. — С. 75-78. — Бібліогр.: 28 назв. — англ.uk_UA
dc.identifier.issn2227-1481
dc.identifier.urihttps://nasplib.isofts.kiev.ua/handle/123456789/119623
dc.language.isoenuk_UA
dc.publisherГоловна астрономічна обсерваторія НАН Україниuk_UA
dc.relation.ispartofAdvances in Astronomy and Space Physics
dc.statuspublished earlieruk_UA
dc.titleV407 Cyg and RS Oph - comparison of two exotic variablesuk_UA
dc.typeArticleuk_UA

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Advances in Astronomy and Space Physics, 2013, вип. 2