Inhomogeneous Chemical Evolution in the Galactic Halo:. Supernova-Induced Formation of Field Stars and Globular Clusters

Details Inhomogeneous Chemical Evolution in the Galactic Halo:. Supernova-Induced Formation of Field Stars and Globular Clusters Inhomogeneous Chemical Evolution in the Galactic Halo:. Supernova-Induced Formation of Field Stars and Globular Clusters

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003omeg.conf...14s&link_type=abstract

ORIGIN OF MATTER AND EVOLUTION OF GALAXIES 2000. Proceedings of the International Symposium. Held 19-21 January 2000 in Universi

Astronomy and Astrophysics

Astronomy

Scientific paper

A model describing the chemical evolution in each cloud of the Galactic halo is presented. The inhomogeneous nature introduced by supernova explosions is incorporated into this model. It is found that if field stars are formed from shells of individual supernova remnants and globular clusters are formed from cloud-cloud collisions the observed metallicity distribution functions of both objects can be reproduced.

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