Note to users. If you're seeing this message, it means that your browser cannot find this page's style/presentation instructions -- or possibly that you are using a browser that does not support current Web standards. Find out more about why this message is appearing, and what you can do to make your experience of our site the best it can be.


Science 30 May 1997:
Vol. 276. no. 5317, pp. 1370 - 1374
DOI: 10.1126/science.276.5317.1370

Articles

Globular Clusters at Low and High Redshift

Denis Burgarella

Globular clusters form homogeneous populations of stars. On the one hand, because initial conditions are homogeneous within one cluster but vary from cluster to cluster, their study can shed light on stellar evolution processes. On the other hand, globular clusters contain the oldest known stellar population in galaxies. The study of the characteristics of globular cluster systems is one way to understand parent galaxy formation and early evolution. Unfortunately, a direct observation of the time when globular clusters and galaxies formed is still out of reach for today's telescopes, but this remains a major goal.

D. Burgarella is in the Laboratoire d'Astronomie Spatiale, Traverse du Siphon, B.P. 8, 13376, Marseille CEDEX 12, France. E-mail: burgarella{at}astrsp-mrs.fr


Read the Full Text


THIS ARTICLE HAS BEEN CITED BY OTHER ARTICLES:
The Baryon Halo of the Milky Way: A Fossil Record of Its Formation.
J. Bland-Hawthorn and K. Freeman (2000)
Science 287, 79-84
   Abstract »    Full Text »



To Advertise     Find Products


Science. ISSN 0036-8075 (print), 1095-9203 (online)