Molecular outflow in the composite galaxy NGC6764
| dc.creator | Leon, Stephane | |
| dc.creator | Eckart, Andreas | |
| dc.creator | Laine, Seppo | |
| dc.creator | Schinnerer, Eva | |
| dc.date | 2002-11-13 | |
| dc.date.accessioned | 2026-07-07T02:06:12Z | |
| dc.date.available | 2026-07-07T02:06:12Z | |
| dc.description | NGC 6764 is a composite galaxy exhibiting central activity (LINER) and recent massive star formation (Wolf-Rayet galaxy). We report new high-resolution interferometric data of the CO(1--0) and CO(2--1) emission in the central part of the galaxy together with high resolution VLA data of the radio continuum emission. The bulk of molecular gas (few times 10^8 Msun) is located in the central part. A molecular outflow (~1.7 x 10^7 Msun) out-of the plane is associated with the starburst-driven outflow radiocontinuum emission. | |
| dc.description | 2 pages, to appear in Active Galactic Nuclei: from Central Engine to Host Galaxy Abstract Book, meeting held in Meudon, France, July 23-27, 2002, Eds.: S. Collin, F. Combes and I. Shlosman (ASP) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0211280 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0211280 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/5339 | |
| dc.subject | Astrophysics | |
| dc.title | Molecular outflow in the composite galaxy NGC6764 | |
| dc.type | text |