No CrossRef data available.
Article contents
The Origin of the Coronal Lines in Seyfert Galaxies
Published online by Cambridge University Press: 07 August 2017
Extract
Photoionization model calculations suggest the possibility that the coronal line region in Seyfert galaxies may be the result of an interstellar medium exposed to and subsequently photoionized by a “bare” Seyfert nucleus. A series of models are presented in which a “generic” AGN continuum illuminates the low-density phase of the ISM of a spiral galaxy (Korista and Ferland 1988).
- Type
- Part 5: Structure of the Central Object and NLR
- Information
- Copyright
- Copyright © Kluwer 1989