Spectroscopic Study of VV Cephei
Observed spectra of the long period eclipsing binary VV Cephei show emission features of Balmer and some ionized metal lines. These features were interpreted as the result of the extended envelope activity surrounding the secondary star. Radial velocities and equivalent widths were calculated from s...
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Korean Space Science Society (KSSS)
1992-06-01
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doaj-c166a169396943938f64395bcc25d44e2020-11-24T22:38:22ZengKorean Space Science Society (KSSS)Journal of Astronomy and Space Sciences2093-55872093-14091992-06-019197110Spectroscopic Study of VV CepheiMun-Suk Chun0Munhwan Gim1Department of Astronomy and Atmospheric Science, Yonsei University, Seoul 120-749, KoreaDepartment of Astronomy and Atmospheric Science, Yonsei University, Seoul 120-749, KoreaObserved spectra of the long period eclipsing binary VV Cephei show emission features of Balmer and some ionized metal lines. These features were interpreted as the result of the extended envelope activity surrounding the secondary star. Radial velocities and equivalent widths were calculated from some metal lines.http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/1992/v9n1/OJOOBS_1992_v9n1_97.pdf |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Mun-Suk Chun Munhwan Gim |
spellingShingle |
Mun-Suk Chun Munhwan Gim Spectroscopic Study of VV Cephei Journal of Astronomy and Space Sciences |
author_facet |
Mun-Suk Chun Munhwan Gim |
author_sort |
Mun-Suk Chun |
title |
Spectroscopic Study of VV Cephei |
title_short |
Spectroscopic Study of VV Cephei |
title_full |
Spectroscopic Study of VV Cephei |
title_fullStr |
Spectroscopic Study of VV Cephei |
title_full_unstemmed |
Spectroscopic Study of VV Cephei |
title_sort |
spectroscopic study of vv cephei |
publisher |
Korean Space Science Society (KSSS) |
series |
Journal of Astronomy and Space Sciences |
issn |
2093-5587 2093-1409 |
publishDate |
1992-06-01 |
description |
Observed spectra of the long period eclipsing binary VV Cephei show emission features of Balmer and some ionized metal lines. These features were interpreted as the result of the extended envelope activity surrounding the secondary star. Radial velocities and equivalent widths were calculated from some metal lines. |
url |
http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/1992/v9n1/OJOOBS_1992_v9n1_97.pdf |
work_keys_str_mv |
AT munsukchun spectroscopicstudyofvvcephei AT munhwangim spectroscopicstudyofvvcephei |
_version_ |
1725713429603287040 |