IMAGES. I. Strong evolution of galaxy kinematics since z = 1

Astronomy and Astrophysics

Volumn 477, Issue 3, 2008, Pages 789-805

  Yang, Y ^a   Flores, H ^a   Hammer, F ^a   Neichel, B ^a   Puech, M ^a,b   Nesvadba, N ^a   Rawat, A ^a,c   Cesarsky, C ^b   Lehnert, M ^a   Pozzetti, L ^d   Fuentes Carrera, I ^a   Amram, P ^e   Balkowski, C ^a   Dannerbauer, H ^f   Di Serego Alighieri, S ^g   Guiderdoni, B ^h   Kembhavi, A ^c   Liang, C ⁱ   Ostlin G ^j   Ravikumar, D ^k   Vergani, D ^l   Vernet, J ^b   Wozniak, H ^h   more..

^a UNIVERSITÉ PARIS DIDEROT   (France)

^b EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^c INTER UNIVERSITY CENTRE FOR ASTRONOMY AND ASTROPHYSICS   (India)

^d OSSERVATORIO ASTRONOMICO DI BOLOGNA   (Italy)

^e AIX MARSEILLE UNIVERSITÉ   (France)

^f MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^g INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

^h CENTRE DE RECHERCHE ASTROPHYSIQUE DE LYON   (France)

ⁱ CHINESE ACADEMY OF SCIENCES   (China)

^j ALBANOVA UNIVERSITY CENTER   (Sweden)

^k UNIVERSITY OF CALICUT   (India)

^l INAF IASF MILANO   (Italy)

more..

Author keywords

Galaxies: evolution; Galaxies: formation; Galaxies: kinematics and dynamics

Indexed keywords

COSMOLOGY; KINEMATICS; SIGNAL TO NOISE RATIO; SPECTROSCOPIC ANALYSIS; STARS;

EMISSION LINES; GALAXIES: EVOLUTION; GALAXIES: FORMATION; GALAXIES: KINEMATICS AND DYNAMICS;

GALAXIES;

EID: 38049112736     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20078219     Document Type: Article

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