| Автор | Lin Qing |
| Автор | Shu Cheng-Gang |
| Автор | Chang Rui-Xiang |
| Автор | Zhao Jun-Liang |
| Дата выпуска | 2001-11-01 |
| dc.description | A model considering gas outflows due to supernova explosions is developed for the star formation and chemical enrichment for the globular clusters (GCs) in the Milky Way galaxy. Through Monte Carlo simulations, the observed global properties of GCs can be well reproduced, including the metallicity distribution, no-correlation between cluster masses and galactocentric distances, etc. The predicted mass function of the parent clouds for the observed GCs at present day can be well described as a power law with the index of -1.8, which is consistent with the current observations for the molecular clouds. |
| Формат | application.pdf |
| Издатель | Institute of Physics Publishing |
| Название | Star Formation and Chemical Enrichment for Globular Clusters |
| Тип | paper |
| DOI | 10.1088/0256-307X/18/11/335 |
| Electronic ISSN | 1741-3540 |
| Print ISSN | 0256-307X |
| Журнал | Chinese Physics Letters |
| Том | 18 |
| Первая страница | 1536 |
| Последняя страница | 1538 |
| Аффилиация | Lin Qing; Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030 |
| Аффилиация | Shu Cheng-Gang; Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030 |
| Аффилиация | Chang Rui-Xiang; Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030 |
| Аффилиация | Zhao Jun-Liang; Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030 |
| Выпуск | 11 |
