High-resolution spectroscopy of the extremely iron-poor post-AGB star CCLyr
文献类型：期刊论文
| 作者 | Aoki, Wako1,2; Matsuno, Tadafumi1,2; Honda, Satoshi3; Parthasarathy, Mudumba4; Li, Haining5 ; Suda, Takuma6
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| 刊名 | PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN
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| 出版日期 | 2017-04-01 |
| 卷号 | 69期号:2 |
| 关键词 | circumstellar matter stars: abundances stars: AGB and post-AGB stars: individual (CC Lyr) |
| 英文摘要 | High-resolution optical spectroscopy was conducted for the metal-poor post-AGB star CC Lyr to determine its chemical abundances and spectral line profiles. Our standard abundance analysis confirms its extremely low metallicity ([Fe/H] < -3.5) and a clear correlation between abundance ratios and the condensation temperature for 11 elements, indicating that dust depletion is the cause of the abundance anomaly of this object. The very low abundances of Sr and Ba, which are detected for the first time for this object, suggest that heavy neutron-capture elements are not significantly enhanced in this object by the s-process during its evolution through the AGB phase. The radial velocity of this object and profiles of some atomic absorption lines show variations depending on pulsation phases, which could be formed by dynamics of the atmosphere rather than by binarity or contributions of circumstellar absorption. On the other hand, the Ha emission with double peaks shows no evident velocity shift, suggesting that the emission is originating from the circumstellar matter, presumably the rotating disk around the object. |
| WOS标题词 | Science & Technology ; Physical Sciences |
| 类目[WOS] | Astronomy & Astrophysics |
| 研究领域[WOS] | Astronomy & Astrophysics |
| 关键词[WOS] | II CEPHEIDS ; CHEMICAL-COMPOSITION ; LOW-MASS ; LAMOST ; ATMOSPHERES ; TELESCOPE ; SCENARIO ; MYSTERY ; CLOUD |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000401118500007 |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/8781]  |
| 专题 | 国家天文台_光学天文研究部 |
| 作者单位 | 1.Natl Astron Observ Japan, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan 2.Grad Univ Adv Studies SOKENDAI, Sch Phys Sci, Dept Astron Sci, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan 3.Univ Hyogo, Ctr Astron, 407-2 Nishigaichi,Sayo Cho, Sayo, Hyogo 6795313, Japan 4.Indian Inst Astrophys, 2 Block, Bangalore 560034, Karnataka, India 5.Chinese Acad Sci, Natl Astron Observ, Key Lab Opt Astron, A20 Datun Rd, Beijing 100012, Peoples R China 6.Univ Tokyo, Res Ctr Early Universe, Bunkyo Ku, 7-3-1 Hongo, Tokyo 1130033, Japan |
| 推荐引用方式 GB/T 7714 | Aoki, Wako,Matsuno, Tadafumi,Honda, Satoshi,et al. High-resolution spectroscopy of the extremely iron-poor post-AGB star CCLyr[J]. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN,2017,69(2). |
| APA | Aoki, Wako,Matsuno, Tadafumi,Honda, Satoshi,Parthasarathy, Mudumba,Li, Haining,&Suda, Takuma.(2017).High-resolution spectroscopy of the extremely iron-poor post-AGB star CCLyr.PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN,69(2). |
| MLA | Aoki, Wako,et al."High-resolution spectroscopy of the extremely iron-poor post-AGB star CCLyr".PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN 69.2(2017). |
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来源：国家天文台
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