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Radio Outflows and the Origin of the Narrow Line Region in Seyfert Galaxies

Published online by Cambridge University Press:  25 May 2016

A. Capetti ,
D.J. Axon ,
F.D. Macchetto  and
W.B. Sparks
A. Capetti
Affiliation:
1 Space Telescope Science Institute - 3700, San Martin Drive, Baltimore, MD 21218, U.S.A.
D.J. Axon
Affiliation:
1 Space Telescope Science Institute - 3700, San Martin Drive, Baltimore, MD 21218, U.S.A.
F.D. Macchetto
Affiliation:
1 Space Telescope Science Institute - 3700, San Martin Drive, Baltimore, MD 21218, U.S.A.
W.B. Sparks
Affiliation:
1 Space Telescope Science Institute - 3700, San Martin Drive, Baltimore, MD 21218, U.S.A.

Extract

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Seven Seyfert galaxies, Mrk 3, Mrk 78, Mrk 348, Mrk 6, Mrk 573, NGC 3393, IRAS 04210+0400 and IRAS 11058-1131 (all Seyfert galaxies type 2 expect Mrk 6 which is a Seyfert 1.5) were observed with HST. For the first five objects images were taken with the FOC with filters centered on the emission lines [O II] and [O III]. For the remaining three galaxies WFPC2 observations were obtained in the [O III] and Hα lines.

Type
Relation between Radio and Other Wavelenghts
Information
Symposium - International Astronomical Union , Volume 175: Extragalactic Radio Sources , 1996 , pp. 230 - 231
Copyright
Copyright © Kluwer 1996