The nature of Lyman-break galaxies.

Details The nature of Lyman-break galaxies. The nature of Lyman-break galaxies.

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999pyuno......196c&link_type=abstract

Publications of the Yunnan Observatory, Suppl. 1999, p. 196 - 203

Physics

Galaxy Clustering: Star Formation

Scientific paper

The number density and clustering properties of Lyman-break galaxies (LBGs) observed at redshift z ≡ 3 are best explained by assuming that they are associated with the most massive haloes at z ≡ 3 predicted in hierarchical models of structure formation. In this paper the authors study, under the same assumption, how star formation and chemical enrichment may have proceeded in the LBG population. They find that gas cooling in dark haloes provides a natural regulation process. The predicted star formation rates and effective radii are consistent with observations.

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