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Kinematical and Spectral Evidences of Complex Structure of NGC 1275 Nucleus

Published online by Cambridge University Press:  04 August 2017

V. I. Pronik*
Affiliation:
Crimean Astrophysical Observatory 334413 p/o Nauchny, Crimea, USSR

Abstract

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The analysis of the available data about spectral observations of nucleus and gas velocity field in NGC 1275 leads to a conclusion on the presence in the nucleus of several spatially separated variable sources responsible for a complex variable emission in Hβ and [OIII] lines profiles.

Type
IV. Variability
Copyright
Copyright © Reidel 1987 

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