Ultraviolet Spectrophotometry of VV Cephei
The IUE archival spectra of VV Cephei were collected to investigate the eclipse nature in the ultraviolet. The temperature of the B star has been determined, as approximately 30000K, based on the flux distributions during egress. Light curves of VV Cephei were reduced from the spectrophotometry of t...
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Korean Space Science Society (KSSS)
1992-06-01
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| Series: | Journal of Astronomy and Space Sciences |
| Online Access: | http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/1992/v9n1/OJOOBS_1992_v9n1_111.pdf |
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doaj-2aaf94b380b24f358ad6caf36b7151d92020-11-24T23:40:42ZengKorean Space Science Society (KSSS)Journal of Astronomy and Space Sciences2093-55872093-14091992-06-0191111119Ultraviolet Spectrophotometry of VV CepheiYoung Woon Kang0Dept. of Earth Science, King Sejong University, Seoul 133-747, KoreaThe IUE archival spectra of VV Cephei were collected to investigate the eclipse nature in the ultraviolet. The temperature of the B star has been determined, as approximately 30000K, based on the flux distributions during egress. Light curves of VV Cephei were reduced from the spectrophotometry of the IUE archival spectra. Three light curves at the center wavelengths of 3250 Å, 2550 Å and 2850 Å have been analyzed by the modified Wilson and Devinney light curve program. The radii of the B star and M star were deduced to 0.05 and 0.22 of unit separation, respectively. The UV light curves show an evidence that the light was attenuated by the highly opaque atomsphere of the M star.http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/1992/v9n1/OJOOBS_1992_v9n1_111.pdf |
| collection |
DOAJ |
| language |
English |
| format |
Article |
| sources |
DOAJ |
| author |
Young Woon Kang |
| spellingShingle |
Young Woon Kang Ultraviolet Spectrophotometry of VV Cephei Journal of Astronomy and Space Sciences |
| author_facet |
Young Woon Kang |
| author_sort |
Young Woon Kang |
| title |
Ultraviolet Spectrophotometry of VV Cephei |
| title_short |
Ultraviolet Spectrophotometry of VV Cephei |
| title_full |
Ultraviolet Spectrophotometry of VV Cephei |
| title_fullStr |
Ultraviolet Spectrophotometry of VV Cephei |
| title_full_unstemmed |
Ultraviolet Spectrophotometry of VV Cephei |
| title_sort |
ultraviolet spectrophotometry 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 |
The IUE archival spectra of VV Cephei were collected to investigate the eclipse nature in the ultraviolet. The temperature of the B star has been determined, as approximately 30000K, based on the flux distributions during egress. Light curves of VV Cephei were reduced from the spectrophotometry of the IUE archival spectra. Three light curves at the center wavelengths of 3250 Å, 2550 Å and 2850 Å have been analyzed by the modified Wilson and Devinney light curve program. The radii of the B star and M star were deduced to 0.05 and 0.22 of unit separation, respectively. The UV light curves show an evidence that the light was attenuated by the highly opaque atomsphere of the M star. |
| url |
http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/1992/v9n1/OJOOBS_1992_v9n1_111.pdf |
| work_keys_str_mv |
AT youngwoonkang ultravioletspectrophotometryofvvcephei |
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