The role of the LIRG and ULIRG phases in the evolution of K\mathsf_s-selected galaxies

2006/04/11 by K. I. Caputi, H. Dole, G. Lagache +5 · 4 citations
Physics and Astronomy · #Astronomy #Astronomy and Astrophysical Research #Astrophysics #Galaxies: Formation, Evolution, Phenomena #Galaxy #Galaxy formation and evolution #Galaxy group #Gamma-ray bursts and supernovae #Luminous infrared galaxy #Physics #astro-ph

paper · pdf · doi:10.1051/0004-6361:20054553

Accepted for publication in A&A. 9 pages, 6 figures

arxiv created 2006/04/11 · arxiv updated 2009/12/01

Abstract

Aims.We investigate the role of the luminous infrared galaxy (LIRG) and ultra-luminous infrared galaxy (ULIRG) phases in the evolution of Ks-selected galaxies and, in particular, Extremely Red Galaxies (ERGs).

Cited by

• Outflows of hot molecular gas in ultra-luminous infrared galaxies mapped with VLT-SINFONI
• Unveiling the Important Role of Groups in the Evolution of Massive Galaxies: Insights from an Infrared Passive Sequence at Intermediate Redshift
• Multiwavelength Study of Massive Galaxies atz∼2. I. Star Formation and Galaxy Growth
• Deep ATCA and VLA Radio Observations of Short-GRB Host Galaxies. Constraints on Star Formation Rates, Afterglow Flux, and Kilonova Radio Flares