| The evolution and star-formation history of M33 | |
Kang XY(康晓宇)1,2,3,4 ; Chang, RX3; Yin, J3; Hou, JL3; Zhang FH(张奉辉)1,2; Zhang Y(张余)1,2,4; Han ZW(韩占文)1,2; Kang, XY (reprint author), Chinese Acad Sci, Yunnan Observ, Natl Astron Observ, Kunming 650011, Peoples R China.
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| 发表期刊 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
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| 2012-10 | |
| 卷号 | 426期号:2页码:1455-1464 |
| DOI | 10.1111/j.1365-2966.2012.21778.x |
| 产权排序 | 第1完成单位 |
| 收录类别 | SCI |
| 关键词 | Galaxies: Abundances Galaxies: Evolution Galaxies: Individual: M33 Galaxies: Spiral |
| 摘要 | We construct a parametrized model to explore the main properties of the star-formation history of M33. We assume that the disc originates and grows by primordial gas infall and adopt a simple form of gas accretion rate with one free parameter, the infall time-scale. We also include the contribution of the gas outflow process. A major update of the model is that we adopt a molecular-hydrogen-correlated star-formation law and calculate the evolution of the atomic and molecular gas separately. Comparisons between the model predictions and observational data show that the model predictions are very sensitive to the adopted infall time-scale, while the gas-outflow process mainly influences the metallicity profile. A model adopting a moderate outflow rate and an inside-out formation scenario can be in good agreement with most of the observed constraints of the M33 disc. We also compare model predictions based on a molecular-hydrogen-correlated star-formation law and that based on the Kennicutt star-formation law. Our results imply that the molecular-hydrogen-correlated star-formation law should be preferred to describe the evolution of the M33 disc, especially the radial distributions of both the cold gas and the stellar population. |
| 项目资助者 | National Natural Science Foundation of China [11273053, 11103058, 11173044, 11033008, 10821061] ; Group Innovation Project [11121062] ; Science Foundation of Shanghai [11ZR1443600] ; Chinese Academy of Sciences ; [10833005] ; [10878003] |
| 语种 | 英语 |
| 学科领域 | Astronomy & Astrophysics |
| 文章类型 | Article |
| ISSN | 0035-8711 |
| URL | 查看原文 |
| 归档日期 | 2012-11-01 |
| WOS记录号 | WOS:000309456200052 |
| WOS研究方向 | Astronomy & Astrophysics |
| WOS类目 | Astronomy & Astrophysics |
| 关键词[WOS] | MASS-METALLICITY RELATION ; NEARBY SPIRAL GALAXIES ; MILKY-WAY DISK ; H-II REGIONS ; ABUNDANCE GRADIENTS ; CHEMICAL EVOLUTION ; PLANETARY-NEBULAE ; GALACTIC DISK ; STELLAR POPULATIONS ; IRREGULAR GALAXIES |
| 引用统计 | |
| 文献类型 | 期刊论文 |
| 条目标识符 | http://ir.ynao.ac.cn/handle/114a53/4521 |
| 专题 | 大样本恒星演化研究组 中国科学院天体结构与演化重点实验室 |
| 通讯作者 | Kang, XY (reprint author), Chinese Acad Sci, Yunnan Observ, Natl Astron Observ, Kunming 650011, Peoples R China. |
| 作者单位 | 1.National Astronomical Observatories, Yunnan Observatory, Chinese Academy of Sciences, Kunming, 650011, China 2.Key Laboratory for the Structure and Evolution of Celestial Objects, Yunnan Astronomical Observatory, Chinese Academy of Sciences, Kunming, 650011, China 3.Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai, 200030, China 4.Graduate School of the Chinese Academy of Sciences, Beijing, 100039, China |
| 第一作者单位 | 中国科学院云南天文台 |
| 推荐引用方式 GB/T 7714 | Kang XY,Chang, RX,Yin, J,et al. The evolution and star-formation history of M33[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2012,426(2):1455-1464. |
| APA | Kang XY.,Chang, RX.,Yin, J.,Hou, JL.,Zhang FH.,...&Kang, XY .(2012).The evolution and star-formation history of M33.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,426(2),1455-1464. |
| MLA | Kang XY,et al."The evolution and star-formation history of M33".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 426.2(2012):1455-1464. |
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| The evolution and st（710KB） | 期刊论文 | 作者接受稿 | 开放获取 | CC BY-NC-SA | 浏览 请求全文 | |
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