Galaxy morphology and evolution from SWAN adaptive optics imaging

Astronomy and Astrophysics

Volumn 458, Issue 2, 2006, Pages 385-396

  Cresci, G ^a   Davies, R I ^b   Baker, A J ^c,d   Mannucci, F ^e   Lehnert, M D ^b   Totani, T ^f   Minowa, Y ^g  

^a INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

^b MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^c NATIONAL RADIO ASTRONOMY OBSERVATORY   (United States)

^d Bldg 142   (United States)

^e CNR   (Italy)

^f KYOTO UNIVERSITY   (Japan)

^g UNIVERSITY OF TOKYO   (Japan)

Author keywords

Galaxies: statistics; Galaxy: fundamental parameters; Infrared: galaxies; Instrumentation: adaptive optics

Indexed keywords

FAINT FIELD GALAXIES; GALAXY FORMATION; GALAXY POPULATION; MORPHOLOGICAL PROPERTIES;

GALAXIES; INFRARED IMAGING; LUMINESCENCE; SATELLITES;

ADAPTIVE OPTICS;

EID: 33750344085     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20065504     Document Type: Article

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