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: | , , , |
| Format: | Artikel |
| Sprache: | English |
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Головна астрономічна обсерваторія НАН України
2013
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| 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 |
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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. |
| work_keys_str_mv |
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| first_indexed |
2025-12-07T13:08:57Z |
| last_indexed |
2025-12-07T13:08:57Z |
| _version_ |
1850855063458676736 |