A SPECTROSCOPICALLY CONFIRMED EXCESS OF 24 μm SOURCES IN A SUPER GALAXY GROUP AT z = 0.37: ENHANCED DUSTY STAR FORMATION RELATIVE TO THE CLUSTER AND FIELD ENVIRONMENT
| dc.creator | Tran, Kim-Vy H. | |
| dc.creator | Saintonge, Amélie | |
| dc.creator | Moustakas, John | |
| dc.creator | Bai, Lei | |
| dc.creator | Gonzalez, Anthony H. | |
| dc.creator | Holden, Bradford P. | |
| dc.creator | Zaritsky, Dennis | |
| dc.creator | Kautsch, Stefan J. | |
| dc.date.accessioned | 2019-10-15T15:56:59Z | |
| dc.date.available | 2019-10-15T15:56:59Z | |
| dc.date.issued | 2009 | |
| dc.identifier.issn | 0004-637X | |
| dc.identifier.issn | 1538-4357 | |
| dc.identifier.uri | https://hdl.handle.net/1969.1/184254 | |
| dc.format.extent | 11 | en |
| dc.publisher | The Astrophysical Journal | |
| dc.relation.ispartof | 1foldr Import 2019-10-08 Batch 13 | en |
| dc.relation.uri | 10.1088/0004-637X/705/1/809 | en |
| dc.title | A SPECTROSCOPICALLY CONFIRMED EXCESS OF 24 μm SOURCES IN A SUPER GALAXY GROUP AT z = 0.37: ENHANCED DUSTY STAR FORMATION RELATIVE TO THE CLUSTER AND FIELD ENVIRONMENT | en |
