36 papers found
Refreshing results…
The MAJORITY OF COMPACT MASSIVE GALAXIES ATz∼ 2 ARE DISK DOMINATED
The Physical Origins of the Morphology-Density Relation: Evidence for Gas Stripping From the Sloan Digital Sky Survey
Major Merging: The Way to Make a Massive, Passive Galaxy
A SPECTROSCOPICALLY CONFIRMED EXCESS OF 24 μm SOURCES IN a SUPER GALAXY GROUP ATz= 0.37: ENHANCED DUSTY STAR FORMATION RELATIVE TO THE CLUSTER AND FIELD ENVIRONMENT
A WIDE-FIELD STUDY OF THEz∼ 0.8 CLUSTER RX J0152.7–1357: THE ROLE OF ENVIRONMENT IN THE FORMATION OF THE RED SEQUENCE
Astronomical Software Wants To Be Free: A Manifesto
Recent Structural Evolution of Early‐Type Galaxies: Size Growth fromz= 1 toz= 0
Spitzer/MIPS 24 μm Observations of Galaxy Clusters: An Increasing Fraction of Obscured Star-forming Members fromz= 0.02 toz= 0.83
Observations of the Gas Reservoir around a Star-Forming Galaxy in the Early Universe
Confirmation of the Remarkable Compactness of Massive Quiescent Galaxies at z ~ 2.3: Early-Type Galaxies Did not Form in a Simple Monolithic Collapse
Looking for the End of Star Formation and the Transformation of Future Cluster Galaxies
Masses and Mass-to-Light Ratios of Early-Type Galaxies at High Redshift ? The Impact of Ultradeep FORS2 Spectroscopy
Life on the Edges: Morphological Transformation of Galaxies in Clusters of Galaxies at z=1
Watching Galaxies Fall into Coma
Measuring Ωmwith theROSATDeep Cluster Survey
The Intracluster Medium inz > 1 Galaxy Clusters
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