Summary on stellar populations
ELTs will bring galaxies within 5 Mpc or more “as close as the Magellanic Clouds”. This is why stellar populations is such an exciting subject for ELTs. We can resolve galaxies into stars and learn their history (1) from the “fossil record” of old stars and (2) looking back in time. The confrontatio...
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Published in | Proceedings of the International Astronomical Union Vol. 1; no. S232; pp. 461 - 463 |
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Main Author | |
Format | Journal Article |
Language | English |
Published |
Cambridge, UK
Cambridge University Press
01.11.2005
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Subjects | |
Online Access | Get full text |
ISSN | 1743-9213 1743-9221 |
DOI | 10.1017/S174392130600113X |
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Summary: | ELTs will bring galaxies within 5 Mpc or more “as close as the Magellanic Clouds”. This is why stellar populations is such an exciting subject for ELTs. We can resolve galaxies into stars and learn their history (1) from the “fossil record” of old stars and (2) looking back in time. The confrontation of these two views will bring important new insights in the star formation history of galaxies and stellar evolution, at the same time. |
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Bibliography: | SourceType-Scholarly Journals-1 ObjectType-Feature-1 content type line 14 |
ISSN: | 1743-9213 1743-9221 |
DOI: | 10.1017/S174392130600113X |