V407 Cygni - nova like outburst in symbiotic system
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, classi...
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| Опубліковано в: : | Advances in Astronomy and Space Physics |
|---|---|
| Дата: | 2012 |
| Автори: | , , |
| Формат: | Стаття |
| Мова: | English |
| Опубліковано: |
Головна астрономічна обсерваторія НАН України
2012
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| Онлайн доступ: | https://nasplib.isofts.kiev.ua/handle/123456789/119182 |
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| Назва журналу: | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| Цитувати: | 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. |
Репозитарії
Digital Library of Periodicals of National Academy of Sciences of Ukraine| id |
nasplib_isofts_kiev_ua-123456789-119182 |
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dspace |
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Drozd, K. Swierczynski, E. Ragan, E. 2017-06-04T18:58:02Z 2017-06-04T18:58:02Z 2012 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. 2227-1481 https://nasplib.isofts.kiev.ua/handle/123456789/119182 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. 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. en Головна астрономічна обсерваторія НАН України Advances in Astronomy and Space Physics V407 Cygni - nova like outburst in symbiotic system Article published earlier |
| institution |
Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| collection |
DSpace DC |
| title |
V407 Cygni - nova like outburst in symbiotic system |
| spellingShingle |
V407 Cygni - nova like outburst in symbiotic system Drozd, K. Swierczynski, E. Ragan, E. |
| title_short |
V407 Cygni - nova like outburst in symbiotic system |
| title_full |
V407 Cygni - nova like outburst in symbiotic system |
| title_fullStr |
V407 Cygni - nova like outburst in symbiotic system |
| title_full_unstemmed |
V407 Cygni - nova like outburst in symbiotic system |
| title_sort |
v407 cygni - nova like outburst in symbiotic system |
| author |
Drozd, K. Swierczynski, E. Ragan, E. |
| author_facet |
Drozd, K. Swierczynski, E. Ragan, E. |
| publishDate |
2012 |
| language |
English |
| container_title |
Advances in Astronomy and Space Physics |
| publisher |
Головна астрономічна обсерваторія НАН України |
| format |
Article |
| description |
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.
|
| issn |
2227-1481 |
| url |
https://nasplib.isofts.kiev.ua/handle/123456789/119182 |
| citation_txt |
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. |
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2025-12-07T20:48:09Z |
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2025-12-07T20:48:09Z |
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