Simulations of early baryonic structure formation with stream velocity. I. Halo abundance

Astrophysical Journal

Volumn 747, Issue 2, 2012, Pages

  Naoz, Smadar ^a   Yoshida, Naoki ^b   Gnedin, Nickolay Y ^c,d,e  

^a NORTHWESTERN UNIVERSITY   (United States)

^b UNIVERSITY OF TOKYO   (Japan)

^c FERMI NATIONAL ACCELERATOR LABORATORY   (United States)

^d UNIVERSITY OF CHICAGO   (United States)

^e UNIVERSITY OF CHICAGO   (United States)

Author keywords

cosmology: theory; early universe; galaxies: formation; galaxies: statistics

Indexed keywords

EID: 84859565522     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/747/2/128     Document Type: Article

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