Hostname: page-component-848d4c4894-r5zm4 Total loading time: 0 Render date: 2024-06-16T12:25:42.571Z Has data issue: false hasContentIssue false
  • English
  • Français

Radio Emission from the Seyfert Galaxy NGC 5548

Published online by Cambridge University Press:  14 August 2015

J. S. Ulvestad ,
A. S. Wilson  and
D. G. Wentzel
J. S. Ulvestad
Affiliation:
NRAO - Charlottesville
A. S. Wilson
Affiliation:
Astronomy Program, University of Maryland
D. G. Wentzel
Affiliation:
Astronomy Program, University of Maryland

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Weak radio emission from the type 1.5 Seyfert galaxy NGC 5548 has been mapped with high resolution at the VLA at both 1465 and 4885 MHz. The galaxy contains the largest (5.9 kpc) triple radio source known in a Seyfert galaxy. The central component of that triple is unresolved (<0.39×0.15 kpc) and has a flatter spectrum than the well-resolved outer lobes. In addition, the field surrounding NGC 5548 and two of the sources in that field have been mapped at 1465 MHz; the field sources are unlikely to be physically associated with NGC 5548.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 97: Extragalactic Radio Sources , 1982 , pp. 191 - 192
Copyright
Copyright © Reidel 1982 

References

de Bruyn, A. G., and Wilson, A. S.: 1978, Astron. Astrophys. 64, pp. 433–444.Google Scholar
Su, H. J., and Simkin, S. M.: 1980, Astrophys. J. 238, pp. L1–L5.CrossRefGoogle Scholar
van der Kruit, P. C.: 1971, Astron. Astrophys. 15, pp. 110–122.Google Scholar
Wilson, A. S., and Willis, A. G.: 1980, Astrophys. J. 240, pp. 429–441.CrossRefGoogle Scholar