V407 Cyg and RS Oph - comparison of two exotic variables

V407 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 thes...

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Veröffentlicht in:Advances in Astronomy and Space Physics
Datum:2013
Hauptverfasser: Drozd, K., Swierczynski, E., Ragan, E., Buil, C.
Format: Artikel
Sprache:English
Veröffentlicht: Головна астрономічна обсерваторія НАН України 2013
Online Zugang:https://nasplib.isofts.kiev.ua/handle/123456789/119623
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Назва журналу:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Zitieren:V407 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.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
id nasplib_isofts_kiev_ua-123456789-119623
record_format dspace
spelling Drozd, K.
Swierczynski, E.
Ragan, E.
Buil, C.
2017-06-07T18:17:29Z
2017-06-07T18:17:29Z
2013
V407 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.
2227-1481
https://nasplib.isofts.kiev.ua/handle/123456789/119623
V407 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.
We 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.
en
Головна астрономічна обсерваторія НАН України
Advances in Astronomy and Space Physics
V407 Cyg and RS Oph - comparison of two exotic variables
Article
published earlier
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
title V407 Cyg and RS Oph - comparison of two exotic variables
spellingShingle V407 Cyg and RS Oph - comparison of two exotic variables
Drozd, K.
Swierczynski, E.
Ragan, E.
Buil, C.
title_short V407 Cyg and RS Oph - comparison of two exotic variables
title_full V407 Cyg and RS Oph - comparison of two exotic variables
title_fullStr V407 Cyg and RS Oph - comparison of two exotic variables
title_full_unstemmed V407 Cyg and RS Oph - comparison of two exotic variables
title_sort v407 cyg and rs oph - comparison of two exotic variables
author Drozd, K.
Swierczynski, E.
Ragan, E.
Buil, C.
author_facet Drozd, K.
Swierczynski, E.
Ragan, E.
Buil, C.
publishDate 2013
language English
container_title Advances in Astronomy and Space Physics
publisher Головна астрономічна обсерваторія НАН України
format Article
description V407 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.
issn 2227-1481
url https://nasplib.isofts.kiev.ua/handle/123456789/119623
citation_txt V407 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.
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