An explanation for the observed weak size evolution of disk galaxies

Astrophysical Journal

Volumn 672, Issue 2, 2008, Pages 776-786

  Somerville, Rachel S ^a   Barden, Marco ^a   Rix, Hans Walter ^a   Bell, Eric F ^a   Beckwith, Steven V W ^b,c   Borch, Andrea ^a,d   Caldwell, John A R ^e   Häußler, Boris ^a   Heymans, Catherine ^f   Jahnke, Knud ^a   Jogee, Shardha ^e   McIntosh, Daniel H ^g   Meisenheimer, Klaus ^a   Peng, Chien Y ^b   Sánchez, Sebastian F ^h   Wisotzki, Lutz ⁱ   Wolf, Christian ^j  

^a MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^b STScI   (United States)

^c JOHNS HOPKINS UNIVERSITY   (United States)

^d ASTRONOMISCHES RECHEN INSTITUT   (Germany)

^e The University of Texas at Austin   (United States)

^f UNIVERSITY OF BRITISH COLUMBIA   (Canada)

^g UNIVERSITY OF MASSACHUSETTS   (United States)

^h Centro Hispano Aleman de Calar Alto   (Spain)

ⁱ ASTROPHYSIKALISCHES INSTITUT POTSDAM   (Germany)

^j UNIVERSITY OF OXFORD   (United Kingdom)

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Author keywords

Cosmology: observations; Galaxies: evolution; Galaxies: high redshift; Galaxies: spiral; Surveys

Indexed keywords

EID: 40249095939     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/523661     Document Type: Article

References (67)