Molecular outflow in the composite galaxy NGC6764

Details Molecular outflow in the composite galaxy NGC6764 Molecular outflow in the composite galaxy NGC6764

2002-11-13

arxiv.org/abs/astro-ph/0211280v1

Astronomy and Astrophysics

Astrophysics

2 pages, to appear in Active Galactic Nuclei: from Central Engine to Host Galaxy Abstract Book, meeting held in Meudon, France

Scientific paper

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.

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