An AST/RO Survey of CO(4-3) in ultracompact HII regions
| dc.creator | Walsh, Wilfred | |
| dc.date | 2003-06-03 | |
| dc.date.accessioned | 2026-07-07T02:08:42Z | |
| dc.date.available | 2026-07-07T02:08:42Z | |
| dc.description | The Antarctic Submillimeter Telescope and Remote Observatory (AST/RO) has been used to observe 78 of the IRAS point sources identified by Bronfman et al. (1996) as likely ultracompact HII regions. Results for the CO(4-3) line at 461.041GHz are presented. The 74 sources detected are bright and in many cases compact, making them potentially suitable as pointing calibrators for single dish submillimeter telescopes. | |
| dc.description | To be submitted to ApJS | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0306075 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0306075 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/6153 | |
| dc.subject | Astrophysics | |
| dc.title | An AST/RO Survey of CO(4-3) in ultracompact HII regions | |
| dc.type | text |