2006/10/05 by Eiichi Egami, E. Egami, G. H. Rieke +3 · 2 citations
Physics and Astronomy · #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Cluster (spacecraft) #Galaxies: Formation, Evolution, Phenomena #Galaxy #Galaxy cluster #Infrared #Luminosity #Luminous infrared galaxy #Physics #Star formation #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.1086/509886
published as Astrophys.J.652:L21-L24,2006 · 13 pages, 3 figures, 1 table; Accepted for publication in ApJL
arxiv created 2006/10/05 · openalex publication_date 2006/10/30 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
We present the Spitzer /IRS mid-infrared spectrum of the infrared-luminous ( L IR = 4 × 10 11 L ☉ ) brightest cluster galaxy (BCG) in the X-ray-luminous cluster Zwicky 3146 (Z3146; z = 0.29). The spectrum shows strong aromatic emission features, indicating that the dominant source of the infrared luminosity is star formation. The most striking feature of the spectrum, however, is the exceptionally strong molecular hydrogen (H 2 ) emission lines, which seem to be shock-excited. The line luminosities and inferred warm H 2 gas mass (~10 10 M ☉ ) are 6 times larger than those of NGC 6240, the most H 2 -luminous galaxy at z ≲ 0.05. Together with the large amount of cold H 2 detected previously (~10 11 M ☉ ), this indicates that the Z3146 BCG contains disproportionately large amounts of both warm and cold H 2 gas for its infrared luminosity, which may be related to the intracluster gas cooling process in the cluster core.