Adaptive Optics Imaging Survey of Luminous Infrared Galaxies
| dc.creator | Laag, Edward A. | |
| dc.creator | Canalizo, Gabriela | |
| dc.creator | van Breugel, Wil | |
| dc.creator | Gates, Elinor L. | |
| dc.creator | de Vries, Wim | |
| dc.creator | Stanford, S. Adam | |
| dc.date | 2006-03-15 | |
| dc.date.accessioned | 2026-07-07T11:25:22Z | |
| dc.date.available | 2026-07-07T11:25:22Z | |
| dc.description | We present high resolution imaging observations of a sample of previously unidentified far-infrared galaxies at z < 0.3. The objects were selected by cross-correlating the IRAS Faint Source Catalog with the VLA FIRST catalog and the HST Guide Star Catalog to allow for adaptive optics observations. We found two new ULIGs (with L_FIR equal to or greater than 10^{12} L_sun) and 19 new LIGs (with L_FIR equal to or greater than 10^{11} L_sun). Twenty of the galaxies in the sample were imaged with either the Lick or Keck adaptive optics systems in H or K'. Galaxy morphologies were determined using the two dimensional fitting program GALFIT and the residuals examined to look for interesting structure. The morphologies reveal that at least 30% are involved in tidal interactions, with 20% being clear mergers. An additional 50% show signs of possible interaction. Line ratios were used to determine powering mechanism; of the 17 objects in the sample showing clear emission lines - four are active galactic nuclei and seven are starburst galaxies. The rest exhibit a combination of both phenomena. | |
| dc.description | 29 pages, 8 figures, accepted for publication in AJ | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0603401 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0603401 | |
| dc.identifier | Astron.J.131:2877-2887,2006 | |
| dc.identifier | doi:10.1086/504112 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/195486 | |
| dc.subject | Astrophysics | |
| dc.title | Adaptive Optics Imaging Survey of Luminous Infrared Galaxies | |
| dc.type | text |