Luminous IR Galaxies in a Merger Sequence: BIMA CO Imaging
| dc.creator | Gao, Yu | |
| dc.creator | Gruendl, R. A. | |
| dc.creator | Hwang, C. -Y. | |
| dc.creator | Lo, K. Y. | |
| dc.date | 1998-12-28 | |
| dc.date.accessioned | 2026-07-07T02:29:50Z | |
| dc.date.available | 2026-07-07T02:29:50Z | |
| dc.description | In order to trace observationally the conditions in the interstellar medium (ISM) that lead to starbursts, we have used the newly expanded Berkeley-Illinois-Maryland Association (BIMA) millimeter-wave array to map the molecular ISM in a sample of LIGs chosen to represent different phases of the interacting/merging process. CO images of 6 galaxy mergers at the early/intermediate stage are shown here and preliminary results are summarized. | |
| dc.description | 4 pages including a postscript figure; talk presentation at IAU Symp. 186 "Galaxy Interactions at Low and High Redshift", J. Barnes & D. Sanders (eds.) in press | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9812459 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9812459 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/13626 | |
| dc.subject | Astrophysics | |
| dc.title | Luminous IR Galaxies in a Merger Sequence: BIMA CO Imaging | |
| dc.type | text |