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Probing active galactic nuclei with H2O megamasers.
We describe the characteristics of the rapidly rotating molecular disk in the nucleus of the mildly active galaxy NGC4258. The morphology and kinematics of the disk are delineated by the point-like watervapor emission sources at 1.35-cm wavelength. High angular resolution [200 microas where as is ar...
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| Main Authors: | , , , , , , |
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| Formáid: | Artigo |
| Teanga: | Inglês |
| Foilsithe: |
1995
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| Ábhair: | |
| Rochtain Ar Líne: | https://ncbi.nlm.nih.gov/pmc/articles/PMC40414/ https://ncbi.nlm.nih.gov/pubmed/11607612 |
| Clibeanna: |
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