Loading...
Please wait, while we are loading the content...
Similar Documents
Star formation histories of resolved galaxies
| Content Provider | Scilit |
|---|---|
| Author | Tosi, Monica |
| Copyright Year | 2008 |
| Description | The colour-magnitude diagrams of resolved stellar populations are the best tool to study the star formation histories of the host galactic regions. In this review the method to derive star formation histories by means of synthetic colour-magnitude diagrams is briefly outlined, and the results of its application to resolved galaxies of various morphological types are summarized. It is shown that all the galaxies studied so far were already forming stars at the lookback time reached by the observational data, independently of morphological type and metallicity. Early-type galaxies have formed stars predominantly, but in several cases not exclusively, at the earliest epochs. All the other galaxies appear to have experienced rather continuous star formation activities throughout their lifetimes, although with significant rate variations and, sometimes, short quiescent phases. |
| Related Links | https://www.cambridge.org/core/services/aop-cambridge-core/content/view/9D3CF1A2CE4179F7C60D8247A345C78E/S1743921309031718a.pdf/div-class-title-star-formation-histories-of-resolved-galaxies-div.pdf |
| Ending Page | 72 |
| Page Count | 12 |
| Starting Page | 61 |
| ISSN | 17439213 |
| e-ISSN | 17439221 |
| DOI | 10.1017/s1743921309031718 |
| Journal | Proceedings of the International Astronomical Union |
| Issue Number | S258 |
| Volume Number | 4 |
| Language | English |
| Publisher | Cambridge University Press (CUP) |
| Publisher Date | 2008-10-01 |
| Access Restriction | Open |
| Subject Keyword | Proceedings of the International Astronomical Union Astronomy and Astrophysics russell Diagram Stellar Content Individual (m31 Leo A) Local Group Magellanic Clouds Evolution |
| Content Type | Text |
| Resource Type | Article |
| Subject | Astronomy and Astrophysics Space and Planetary Science |
