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The Astrophysical Journal Supplement Series
Article . 2001 . Peer-reviewed
Data sources: Crossref
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https://dx.doi.org/10.48550/ar...
Article . 2000
License: arXiv Non-Exclusive Distribution
Data sources: Datacite
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Jet Directions in Seyfert Galaxies: Radio Continuum Imaging Data

Authors: Schmitt, H. R.; Ulvestad, J. S.; Antonucci, R. R. J.; Kinney, A. L.;

Jet Directions in Seyfert Galaxies: Radio Continuum Imaging Data

Abstract

We present the results of VLA A-array 8.46 GHz continuum imaging of 55 Seyfert galaxies (19 Seyfert 1's and 36 Seyfert 2's). These galaxies are part of a larger sample of 88 Seyfert galaxies, selected from mostly isotropic properties, the flux at 60 mum and warm infrared 25 mum to 60 mum colors. These images are used to study the structure of the radio continuum emission of these galaxies and their position angles, in the case of extended sources. These data, combined with information from broad-band B and I observations, have been used to study the orientation of radio jets relative to the plane of their host galaxies (Kinney et al. 2000).

To appear in The Astrophysical Journal Supplement Series, February 2001, 14 pages, 1 figure (6 pages), 2 tables

Keywords

Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
87
Top 10%
Top 10%
Top 10%
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gold