Circumnuclear emission line regions in Cygnus A

  • I. Pérez-Fournon*
  • , F. Cabrera-Guerra
  • , J. Burgos-Martin
  • , J. A. Acosta-Pulido
  • , A. S. Wilson
  • , Z. Tsvetanov
  • *Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

Abstract

We have used the Nordic Optical and the William Herschel Telescopes to obtain images and long-slit spectra of Cygnus A under conditions of sub-arcsecond seeing. The high spatial resolution and accurate positional information obtained from a comparison between the images and spectra allow us to study in detail the kinematics and excitation of the extended ionized gas. Strong velocity gradients and complex line profiles are detected in positions close to the radio axis corresponding to the emission line clouds recently resolved by HST. The results are interpreted in terms of a strong interaction between the radio jet and the interstellar medium.

Original languageEnglish
Pages (from-to)51-55
Number of pages5
JournalVistas in Astronomy
Volume40
Issue number1
DOIs
Publication statusPublished - 1996
Externally publishedYes

Fingerprint

Dive into the research topics of 'Circumnuclear emission line regions in Cygnus A'. Together they form a unique fingerprint.

Cite this