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A slow merger history of field galaxies since z ∼ 1
K Bundy et al.
ASTROPHYSICAL JOURNAL (2004)
Galaxy pairs in the 2dF survey - II. Effects of interactions on star formation in groups and clusters
MS Alonso et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2004)
Star formation in close pairs selected from the Sloan Digital Sky Survey
B Nikolic et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2004)
The DEEP2 Galaxy Redshift Survey:: Evolution of close galaxy pairs and major-merger rates up to z∼1.2
LW Lin et al.
ASTROPHYSICAL JOURNAL (2004)
Unequal-mass galaxy merger remnants: Spiral-like morphology but elliptical-like kinematics
F Bournaud et al.
ASTRONOMY & ASTROPHYSICS (2004)
Galaxy pairs in the 2dF survey - I. Effects of interactions on star formation in the field
DG Lambas et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2003)
Statistical properties of collisionless equal- and unequal-mass merger remnants of disk galaxies
T Naab et al.
ASTROPHYSICAL JOURNAL (2003)
Double starbursts triggered by mergers in hierarchical clustering scenarios
PB Tissera et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2002)
Dynamically close galaxy pairs and merger rate evolution in the CNOC2 redshift survey
DR Patton et al.
ASTROPHYSICAL JOURNAL (2002)
Populating a cluster of galaxies -: I.: Results at z=0
V Springel et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2001)
The origin of star formation gradients in rich galaxy clusters
ML Balogh et al.
ASTROPHYSICAL JOURNAL (2000)
New techniques for relating dynamically close galaxy pairs to merger and accretion rates: Application to the Second Southern Sky Redshift Survey
DR Patton et al.
ASTROPHYSICAL JOURNAL (2000)
Tidally triggered star formation in close pairs of galaxies
EJ Barton et al.
ASTROPHYSICAL JOURNAL (2000)
Hubble Space Telescope imaging of the CFRS and LDSS redshift surveys -: IV.: Influence of mergers in the evolution of faint field galaxies from z∼1
O Le Fèvre et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2000)