In:
Symposium - International Astronomical Union, Cambridge University Press (CUP), Vol. 207 ( 2002), p. 196-198
Kurzfassung:
Washington CCD photometry of intermediate-age clusters in the Small Magellanic Cloud (SMC) is presented. The cluster age distribution in the SMC suggests formation epochs at 3 and 6 Gyr, respectively. Recent star formation is confined to the central body of the SMC. The chemical evolution of the SMC appears to be best represented by bursty models.
Materialart:
Online-Ressource
ISSN:
0074-1809
DOI:
10.1017/S0074180900223735
Sprache:
Englisch
Verlag:
Cambridge University Press (CUP)
Publikationsdatum:
2002
SSG:
16,12