A forming, dust-enshrouded disk at z = 0.43: The first example of a massive, late-type spiral rebuilt after a major merger?

Astronomy and Astrophysics

Volumn 496, Issue 2, 2009, Pages 381-387

  Hammer, F ^a   Flores, H ^a   Yang, Y B ^a   Athanassoula, E ^b   Puech, M ^a,c   Rodrigues, M ^a   Peirani, S ^d  

^a OBSERVATOIRE DE PARIS   (France)

^b AIX MARSEILLE UNIVERSITÉ   (France)

^c EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^d INSTITUT D'ASTROPHYSIQUE DE PARIS   (France)

Author keywords

Galaxies: Formation; Galaxies: Spiral; Galaxy: Kinematics and dynamics

Indexed keywords

ANGULAR MOMENTUM; COSMOLOGY; DISKS (STRUCTURAL COMPONENTS); DUST; DYNAMICS; FORMING; KINEMATICS; MERGERS AND ACQUISITIONS; MERGING; STARS;

COMBINED SYSTEMS; COSMIC STARS; GALAXIES: FORMATION; GALAXIES: SPIRAL; GALAXY: KINEMATICS AND DYNAMICS; HIGH VELOCITIES; LATE TYPES; MILKY WAYS; OUTFLOW MECHANISMS; PHYSICAL MODELS; RAPID EVOLUTIONS; SPIRAL ARMS; SUB-COMPONENTS;

GALAXIES;

EID: 62749142594     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200810488     Document Type: Article

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