English

The extended narrow line region in Mkn79. I.Observations

Astrophysics 2007-05-23 v1

Abstract

We present deep long slit spectra of Mkn79 in position angles PA=12o^{o} and PA=50o^{o} obtained with the WHT. These data prove the existence of an extended narrow line region in PA=12o^{o}, which coincides with the triplet radio structure (Ulvestad \& Wilson 1984) and the observed outflow of material from the nucleus at PA=10o^{o} (Whittle et al. 1988). The ratios of the high to low ionization lines indicate a higher level of gas excitation in PA=12o^{o} compared to PA=50o^{o}. The [NII]λ\lambda6583/Hα\alpha and [SII]λ\lambda6717,31/Hα\alpha versus [OIII]λ\lambda5007/Hβ\beta line ratios are consistent with excitation by an AGN continuum rather than a HII region.

Keywords

Cite

@article{arxiv.astro-ph/9509097,
  title  = {The extended narrow line region in Mkn79. I.Observations},
  author = {L. S. Nazarova and P. T. O'Brien and M. J. Ward},
  journal= {arXiv preprint arXiv:astro-ph/9509097},
  year   = {2007}
}

Comments

uuencoded compressed postscript. The preprint is also available at http://www.ast.cam.ac.uk/preprint/PrePrint.html