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Molecule Formation in the Seyfert Galaxy NGC 1068
Published online by Cambridge University Press: 14 August 2015
Abstract
We have constructed models of relatively high-density radiation-bounded filaments near the nucleus of a Seyfert 2 galaxy. The amount of molecular hydrogen predicted by the models for reasonable values of the physical parameters is consistent with observations of the infrared continuum and the quadrupole rotation-vibration lines of H2 in NGC 1068.
- Type
- Research Article
- Information
- Symposium - International Astronomical Union , Volume 87: Interstellar Molecules , 1980 , pp. 471 - 472
- Copyright
- Copyright © Reidel 1980