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American Astronomical Society, Astrophysical Journal, 1(705), p. 809-820, 2009

DOI: 10.1088/0004-637x/705/1/809

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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

Journal article published in 2009 by Kim-Vy H. Tran ORCID, Amélie Saintonge ORCID, John Moustakas ORCID, Lei Bai, Anthony H. Gonzalez, Bradford P. Holden, Dennis Zaritsky, Stefan J. Kautsch
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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