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Molecule Formation in the Seyfert Galaxy NGC 1068

Published online by Cambridge University Press:  14 August 2015

Wayne J. Carlson  and
Craig B. Foltz
Wayne J. Carlson
Affiliation:
The Ohio State University, Columbus, Ohio
Craig B. Foltz
Affiliation:
The Ohio State University, Columbus, Ohio

Abstract

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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 

References

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