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Physical properties of simulated galaxy populations at z = 2 - I. Effect of metal-line cooling and feedback from star formation and AGN (2013)

First Author: Haas M

Attributed to: Visiting Fellowships at Durham funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stt1487

Publication URI: http://dx.doi.org/10.1093/mnras/stt1487

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 4