A more powerful evolution model for rotating stars
文献类型：期刊论文
| 作者 | Ceng YR(曾艺蓉)
|
| 刊名 | ASTRONOMY & ASTROPHYSICS
 |
| 出版日期 | 2002-11 |
| 卷号 | 394期号:3页码:965-969 |
| 关键词 | stars : evolution stars : rotation stars : Hertzsprung-Russell (HR) and C-M diagrams |
| ISSN号 | 0004-6361 |
| 产权排序 | 第一完成单位 |
| 通讯作者 | Zeng, YR (reprint author), Yunnan Astron Observ, POB 110, Kunming 650011, Peoples R China. |
| 英文摘要 | A new one-dimensional rotating stellar evolution model was developed which, distinct from its previous counterparts based on a conservative rotation case or a "shellular rotation" case, made no special assumptions on the distribution of angular velocity inside a rotating star. The results of the evolutionary calculations are presented and compared with the results of previous studies. |
| 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] | A-TYPE SUPERGIANTS ; WOLF-RAYET STARS ; LOW-MASS STARS ; MICROSCOPIC DIFFUSION ; STELLAR EVOLUTION ; ANGULAR-MOMENTUM ; OB STARS ; ABUNDANCES ; PARAMETERS ; OPACITIES |
| 收录类别 | SCI ; EI |
| 原文出处 | http://www.aanda.org/articles/aa/abs/2002/42/aa2746/aa2746.html |
| 语种 | 英语 |
| WOS记录号 | WOS:000178885000023 |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/5157]  |
| 专题 | 云南天文台_恒星物理研究组 |
| 作者单位 | Yunnan Astronomical Observatory and National Astronomical Observatories, PO Box 110, 650011 Kunming, PR China |
| 推荐引用方式 GB/T 7714 | Ceng YR. A more powerful evolution model for rotating stars[J]. ASTRONOMY & ASTROPHYSICS,2002,394(3):965-969. |
| APA | Ceng YR.(2002).A more powerful evolution model for rotating stars.ASTRONOMY & ASTROPHYSICS,394(3),965-969. |
| MLA | Ceng YR."A more powerful evolution model for rotating stars".ASTRONOMY & ASTROPHYSICS 394.3(2002):965-969. |
入库方式： OAI收割
来源：云南天文台
浏览0
下载0
收藏0
其他版本
除非特别说明，本系统中所有内容都受版权保护，并保留所有权利。