Gas Dynamics in the Luminous Merger NGC 6240
We report 0.5"x0.9" resolution, interferometric observations of the 1.3 mm CO J=2-1 line in the infrared luminous galactic merger NGC 6240. About half of the CO flux is concentrated in a rotating but highly turbulent, thick disk structure centered between the two radio and near-infrared nu...
| Hauptverfasser: | , , , , , |
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| Format: | Journal article |
| Sprache: | English |
| Veröffentlicht: |
Institute of Physics Publishing
1999
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