High-dispersion H alpha spectroscopy of epsilon Aurigae
文献类型:期刊论文
作者 | Cha GW(茶光伟)![]() ![]() ![]() ![]() |
刊名 | ASTRONOMY & ASTROPHYSICS
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出版日期 | 1994-04 |
卷号 | 284期号:3页码:874-882 |
关键词 | STAR, EPSILON-AURIGAE-SPECTROSCOPIC BINARIES STARS, SUPERGIANTS STARS, CIRCUMSTELLAR MATTER |
ISSN号 | 0004-6361 |
产权排序 | 第一完成单位 |
通讯作者 | CHA, GW |
英文摘要 | Halpha spectroscopic observations have been made by using a high-dispersion and high-resolution thick CCD system, when the orbital phase of epsilon Aur was near 0.3. During two years of out-of-eclipse observations, the Halpha profile varied significantly. The circumstellar gas circling the F0 supergiant is possibly a ring-like H II structure, which consists of moving gaseous clouds. Halpha profile variation outside eclipse may be due to the apparent motion of gaseous clouds within the ring following the rotation of the primary, and to its intrinsic physical changes. |
WOS标题词 | Science & Technology ; Physical Sciences |
学科主题 | Astronomy & Astrophysics |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | Astronomy & Astrophysics |
关键词[WOS] | STAR, EPSILON-AURIGAE-SPECTROSCOPIC BINARIES ; STARS, SUPERGIANTS ; STARS, CIRCUMSTELLAR MATTER |
收录类别 | SCI |
原文出处 | http://adsabs.harvard.edu/abs/1994A%26A...284..874C |
语种 | 英语 |
WOS记录号 | WOS:A1994NJ38500016 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/5137] ![]() |
专题 | 云南天文台_恒星物理研究组 |
作者单位 | Yunnan Observatory, P.O. Box 110, Kunming, People's Republic of China |
推荐引用方式 GB/T 7714 | Cha GW,Tan HS,Xu J,et al. High-dispersion H alpha spectroscopy of epsilon Aurigae[J]. ASTRONOMY & ASTROPHYSICS,1994,284(3):874-882. |
APA | Cha GW,Tan HS,Xu J,&Li YS.(1994).High-dispersion H alpha spectroscopy of epsilon Aurigae.ASTRONOMY & ASTROPHYSICS,284(3),874-882. |
MLA | Cha GW,et al."High-dispersion H alpha spectroscopy of epsilon Aurigae".ASTRONOMY & ASTROPHYSICS 284.3(1994):874-882. |
入库方式: OAI收割
来源:云南天文台
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