| The nuclear diversity of Type Ia supernova explosions | |
Podsiadlowski, Philipp1; Mazzali, Paolo2,3; Lesaffre, Pierre1,4,5; Han ZW(韩占文)6 ; Foerster, Francisco1; Podsiadlowski, P (reprint author), Univ Oxford, Dept Astrophys, Keble Rd, Oxford OX1 3RH, England.
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| 2008-10 | |
| 会议名称 | 6th International Conference on Astronomy with Radioactivities |
| 会议录名称 | NEW ASTRONOMY REVIEWS |
| 卷号 | 52 |
| 期号 | 7-10 |
| 页码 | 381-385 |
| 会议日期 | 2008-01-07 |
| 会议地点 | Kreuth, GERMANY |
| 出版地 | THE BOULEVARD, LANGFORD LANE, KIDLINGTON, OXFORD OX5 1GB, OXON, ENGLAND |
| 出版者 | ELSEVIER SCI LTD |
| 产权排序 | 第6完成单位 |
| 摘要 | While Type Ia supernovae (SNe Ia) have been successfully used as cosmological distance candles, there is a large diversity of explosion properties that is presently not understood, nor how this diversity is linked to the properties of their progenitors. Here we review the present status of our understanding of SN Ia progenitors, the main classes of progenitor models and recent observational constraints, the origin of the lightcurve peak - lightcurve width relation (the 'Phillips relation') and its metallicity dependence, and illustrate how different evolutionary histories produce a diversity of pre-supernova properties. We particularly emphasize the importance of the final carbon simmering phase preceding the final runaway and the role of the convective Urca process which will alter the immediate pre-supernova conditions in the exploding white dwarf. (C) 2008 Elsevier B.V. All rights reserved. |
| 关键词 | Binaries: Close Cosmological Parameters Nuclear Reactions Nucleosynthesis Abundances Supernovae: Type Ia White Dwarfs |
| 学科领域 | Astronomy & Astrophysics |
| DOI | 10.1016/j.newar.2008.06.020 |
| URL | 查看原文 |
| 收录类别 | SCI ; CPCI |
| ISSN号 | 1387-6473 |
| 语种 | 英语 |
| WOS研究方向 | Astronomy & Astrophysics |
| WOS标题词 | Science & Technology ; Physical Sciences |
| WOS类目 | Astronomy & Astrophysics |
| WOS记录号 | WOS:000260738300007 |
| 关键词[WOS] | X-RAY SOURCES ; CONVECTIVE URCA PROCESS ; DOUBLE WHITE-DWARFS ; CLOSE BINARIES ; EVOLUTION ; MODELS ; PROGENITORS ; DEGENERATE ; SYSTEMS ; STAR |
| 引用统计 | |
| 文献类型 | 会议论文 |
| 条目标识符 | http://ir.ynao.ac.cn/handle/114a53/236 |
| 专题 | 大样本恒星演化研究组 |
| 通讯作者 | Podsiadlowski, P (reprint author), Univ Oxford, Dept Astrophys, Keble Rd, Oxford OX1 3RH, England. |
| 作者单位 | 1.Department of Astrophysics, University of Oxford, Keble Road, Oxford OX1 3RH, United Kingdom 2.Max-Planck Institut für Astrophysik, Karl-Schwarzschildstr. 1, 85748 Garching, Germany 3.Istituto Naz. di Astrofisica-Oss. Astron., Via Tiepolo, 11, 34131 Trieste, Italy 4.LERMA, CNRS UMR8112, Observatoire de Paris and ENS/LRA, 24 rue Lhomond, 75231 Paris Cedex 05, France 5.Institute of Astronomy, Madingley Road, Cambridge CB3 0HA, United Kingdom 6.National Astronomy Observatories, Yunnan Observatory, The Chinese Academy of Sciences, P.O. Box, Kunming 650011, China |
| 推荐引用方式 GB/T 7714 | Podsiadlowski, Philipp,Mazzali, Paolo,Lesaffre, Pierre,et al. The nuclear diversity of Type Ia supernova explosions[C]. THE BOULEVARD, LANGFORD LANE, KIDLINGTON, OXFORD OX5 1GB, OXON, ENGLAND:ELSEVIER SCI LTD,2008:381-385. |
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| 文件名称/大小 | 文献类型 | 版本类型 | 开放类型 | 使用许可 | ||
| The nuclear diversit（307KB） | 会议论文 | 开放获取 | CC BY-NC-SA | 请求全文 | ||
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