| Asteroseismology of the ZZ Ceti and DAZ GD 133 | |
Fu, JN1; Vauclair, G2,3; Su, J1 ; Cang, T1; Li, C1; Xue, H1; Jiang, XJ5; Li Y(李焱)4; Niu, H6; Zhang, X6; Colas, F7; Dolez, N2,3; Machado, LF8; Michel, R8; Alvarez, M8; Kim, SL9
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| 会议录名称 | Astronomical Society of the Pacific (ASP) Conference Series - 20TH EUROPEAN WHITE DWARF WORKSHOP |
| 2017 | |
| 卷号 | 509 |
| 页码 | 355-358 |
| 会议录编者/会议主办者 | Tremblay, PE; Gansicke, B; Marsh, T |
| 产权排序 | 第4完成单位 |
| 收录类别 | CPCI |
| 会议名称 | 20th European Workshop on White Dwarfs (EuroWD) |
| 会议日期 | 2016-07-25 |
| 会议地点 | Univ Warwick, Coventry, UNITED KINGDOM |
| 会议赞助商 | European Res Council |
| 摘要 | GD 133 is a DAZ white dwarf with an atmosphere polluted by heavy elements accreted from a debris disk, which is formed by the disruption of rocky planetesimals with orbits bringing them at the white dwarf tidal radius. To reach such orbits implies the potential presence of a perturbing planet. GD 133 is a ZZ Ceti pulsator close to the blue edge of the instability strip. The presence of a planet could be revealed by the periodical variation of the observed pulsation periods induced by the orbital motion of the white dwarf around the barycenter of the system. We started a multi-site photometric follow-up aimed at detecting the signature of this potential planet. As a preliminary result of this work in progress, we give the parameters of the GD 133 best-fit model derived from asteroseismology. |
| 资助项目 | N/A |
| 项目资助者 | N/A |
| 语种 | 英语 |
| 学科领域 | 天文学 |
| 文章类型 | Proceedings Paper |
| 出版者 | ASTRONOMICAL SOC PACIFIC |
| 出版地 | 390 ASHTON AVE, SAN FRANCISCO, CA 94112 USA |
| ISBN号 | 978-1-58381-902-9 |
| ISSN号 | 1050-3390 |
| URL | 查看原文 |
| WOS记录号 | WOS:000401592100059 |
| WOS研究方向 | Astronomy & Astrophysics |
| WOS类目 | Astronomy & Astrophysics |
| 关键词[WOS] | Stellar Astrophysics Mesa ; White-dwarfs ; Modules ; Planets |
| 引用统计 | |
| 文献类型 | 会议论文 |
| 条目标识符 | http://ir.ynao.ac.cn/handle/114a53/10039 |
| 专题 | 恒星物理研究组 |
| 通讯作者 | Fu, JN |
| 作者单位 | 1.Department of Astronomy, Beijing Normal University, 100875 Beijing, China 2.Université de Toulouse, UPS-OMP, IRAP, Toulouse, France 3.CNRS, IRAP, 14 avenue Edouard Belin, F-31400 Toulouse, France 4.Yunnan Observatories, Chinese Academy of Sciences, P.O. Box 110, Kunming, 650011, China 5.National Astronomical Observatories, Chinese Academy of Sciences, 20A, Datun Road, Chaoyang District, 100012 Beijing, China 6.Xinjiang Astronomical Observatory, Chinese Academy of Sciences, Urumqi, 830011, China 7.IMCCE, Observatoire de Paris, UMR 8028 CNRS, F-75014 Paris, France 8.Instituto de Astronomía, Observatorio Astronómico Nacional San Pedro, Martir, Universidad Nacional Autónoma de México, 22860 Ensenada, Baja, California, México 9.Korea Astronomy and Space Science Institute, San 61-1, Hwaan, Yuseong, 305-348 Daejeon, Korea |
| 推荐引用方式 GB/T 7714 | Fu, JN,Vauclair, G,Su, J,et al. Asteroseismology of the ZZ Ceti and DAZ GD 133[C]//Tremblay, PE; Gansicke, B; Marsh, T. 390 ASHTON AVE, SAN FRANCISCO, CA 94112 USA:ASTRONOMICAL SOC PACIFIC,2017:355-358. |
| 条目包含的文件 | ||||||
| 文件名称/大小 | 文献类型 | 版本类型 | 开放类型 | 使用许可 | ||
| Asteroseismology of （202KB） | 会议论文 | 开放获取 | CC BY-NC-SA | 浏览 请求全文 | ||
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