The evolution of the spiral galaxy M51a
文献类型：会议论文
| 作者 | Kang XY(康晓宇)1 ; Zhang FH(张奉辉)1; Chang, RX2
|
| 出版日期 | 2015-09-15 |
| 会议名称 | 319th IAU Symposium - Galaxies at High Redshift and Their Evolution Over Cosmic Time |
| 会议日期 | 2015-08-11 |
| 会议地点 | Honolulu, United States |
| 关键词 | galaxies: abundance galaxies: evolution galaxies: individual: M51a galaxies: spiral |
| 卷号 | 319 |
| 页码 | 129-129 |
| 英文摘要 | A simple model for M51a is constructed to explore its evolutionary history by assuming its disk grows from continuous gas infall, which is shaped by a free parameter-the infall-peak time t p. By adopting a constant infall-peak time t p = 7.0Gyr, our model predictions can reproduce most of the observed constraints and still show that the disk of M51a forms inside-out. Our results also show that the current molecular gas surface density, the star-formation rate and the UV-band surface brightness are important quantities to trace the effect of recent interactions on galactic star-formation process. |
| 收录类别 | 其他 |
| 产权排序 | 第一完成单位 |
| 会议网址 | http://adsabs.harvard.edu/abs/2016IAUS..319..129K |
| 会议录 | Proceedings of International Astronomical Union (IAU) Symposium - Galaxies at High Redshift and Their Evolution Over Cosmic Time
 |
| 会议录出版者 | Cambridge University Press |
| 学科主题 | 天文学 |
| 语种 | 英语 |
| ISBN号 | 9781107138261 |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/9779]  |
| 专题 | 云南天文台_大样本恒星演化研究组 |
| 作者单位 | 1.Yunnan Observatories, CAS, Kunming, 650011, China 2.Key Laboratory for Research in Galaxies and Cosmology, Shangahi Astronomical Observatory, CAS, 80 Nandan Road, Shanghai, 200030, China |
| 推荐引用方式 GB/T 7714 | Kang XY,Zhang FH,Chang, RX. The evolution of the spiral galaxy M51a[C]. 见:319th IAU Symposium - Galaxies at High Redshift and Their Evolution Over Cosmic Time. Honolulu, United States. 2015-08-11.http://adsabs.harvard.edu/abs/2016IAUS..319..129K. |
入库方式： OAI收割
来源：云南天文台
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