Low-resolution spectroscopy of the chromospherically active stars 61 Cyg AB with small telescopes
We carried out high-speed low-resolution spectroscopy of two stars, 61 Cyg A and B with small telescopes. They are known as chromospherically active stars of the K5V (A) and K7V (B) spectral types. These two stars are supposed to have high-powered chromospheres. Spectroscopic monitoring of both star...
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| Опубліковано в: : | Advances in Astronomy and Space Physics |
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| Дата: | 2014 |
| Автори: | , , , |
| Формат: | Стаття |
| Мова: | English |
| Опубліковано: |
Головна астрономічна обсерваторія НАН України
2014
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| Онлайн доступ: | https://nasplib.isofts.kiev.ua/handle/123456789/119806 |
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| Назва журналу: | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| Цитувати: | Low-resolution spectroscopy of the chromospherically active stars 61 Cyg AB with small telescopes / S.M. Pokhvala, B.E. Zhilyaev, V.M. Reshetnyk, V.I. Shavlovskij // Advances in Astronomy and Space Physics. — 2014. — Т. 4., вип. 1-2. — С. 25-27. — Бібліогр.: 5 назв. — англ. |
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Digital Library of Periodicals of National Academy of Sciences of Ukraine| id |
nasplib_isofts_kiev_ua-123456789-119806 |
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dspace |
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Pokhvala, S.M. Zhilyaev, B.E. Reshetnyk, V.M. Shavlovskij, V.I. 2017-06-09T19:42:04Z 2017-06-09T19:42:04Z 2014 Low-resolution spectroscopy of the chromospherically active stars 61 Cyg AB with small telescopes / S.M. Pokhvala, B.E. Zhilyaev, V.M. Reshetnyk, V.I. Shavlovskij // Advances in Astronomy and Space Physics. — 2014. — Т. 4., вип. 1-2. — С. 25-27. — Бібліогр.: 5 назв. — англ. 2227-1481 DOI: 10.17721/2227-1481.4.25-27 https://nasplib.isofts.kiev.ua/handle/123456789/119806 We carried out high-speed low-resolution spectroscopy of two stars, 61 Cyg A and B with small telescopes. They are known as chromospherically active stars of the K5V (A) and K7V (B) spectral types. These two stars are supposed to have high-powered chromospheres. Spectroscopic monitoring of both stars showed variations of intensity in the Balmer lines and the Mg b triplets at time intervals ranging from seconds to several minutes. From the spectrum data one can find that relative variations in the Hα, Hβ lines and the Mg b triplets are about 1% and the relative power of chromospheric activity about 2 · 10⁻⁴. en Головна астрономічна обсерваторія НАН України Advances in Astronomy and Space Physics Low-resolution spectroscopy of the chromospherically active stars 61 Cyg AB with small telescopes Article published earlier |
| institution |
Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| collection |
DSpace DC |
| title |
Low-resolution spectroscopy of the chromospherically active stars 61 Cyg AB with small telescopes |
| spellingShingle |
Low-resolution spectroscopy of the chromospherically active stars 61 Cyg AB with small telescopes Pokhvala, S.M. Zhilyaev, B.E. Reshetnyk, V.M. Shavlovskij, V.I. |
| title_short |
Low-resolution spectroscopy of the chromospherically active stars 61 Cyg AB with small telescopes |
| title_full |
Low-resolution spectroscopy of the chromospherically active stars 61 Cyg AB with small telescopes |
| title_fullStr |
Low-resolution spectroscopy of the chromospherically active stars 61 Cyg AB with small telescopes |
| title_full_unstemmed |
Low-resolution spectroscopy of the chromospherically active stars 61 Cyg AB with small telescopes |
| title_sort |
low-resolution spectroscopy of the chromospherically active stars 61 cyg ab with small telescopes |
| author |
Pokhvala, S.M. Zhilyaev, B.E. Reshetnyk, V.M. Shavlovskij, V.I. |
| author_facet |
Pokhvala, S.M. Zhilyaev, B.E. Reshetnyk, V.M. Shavlovskij, V.I. |
| publishDate |
2014 |
| language |
English |
| container_title |
Advances in Astronomy and Space Physics |
| publisher |
Головна астрономічна обсерваторія НАН України |
| format |
Article |
| description |
We carried out high-speed low-resolution spectroscopy of two stars, 61 Cyg A and B with small telescopes. They are known as chromospherically active stars of the K5V (A) and K7V (B) spectral types. These two stars are supposed to have high-powered chromospheres. Spectroscopic monitoring of both stars showed variations of intensity in the Balmer lines and the Mg b triplets at time intervals ranging from seconds to several minutes. From the spectrum data one can find that relative variations in the Hα, Hβ lines and the Mg b triplets are about 1% and the relative power of chromospheric activity about 2 · 10⁻⁴.
|
| issn |
2227-1481 |
| url |
https://nasplib.isofts.kiev.ua/handle/123456789/119806 |
| citation_txt |
Low-resolution spectroscopy of the chromospherically active stars 61 Cyg AB with small telescopes / S.M. Pokhvala, B.E. Zhilyaev, V.M. Reshetnyk, V.I. Shavlovskij // Advances in Astronomy and Space Physics. — 2014. — Т. 4., вип. 1-2. — С. 25-27. — Бібліогр.: 5 назв. — англ. |
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2025-11-30T11:05:23Z |
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