Constraining dark matter halo profiles and galaxy formation models using spiral arm morphology. I. Method outline

Astrophysical Journal

Volumn 645, Issue 2 I, 2006, Pages 1012-1023

  Seigar, Marc S ^a   Bullock, James S ^a   Barth, Aaron J ^a   Ho, Luis C ^b  

^a UNIVERSITY OF CALIFORNIA   (United States)

^b CARNEGIE OBSERVATORIES   (United States)

Author keywords

Dark matter; Galaxies: Fundamental parameters; Galaxies: Halos; Galaxies: Kinematics and dynamics; Galaxies: Spiral; Galaxies: Structure

Indexed keywords

EID: 33746881426     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/504463     Document Type: Article

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