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=12 and PA=50 obtained with the WHT. These data prove the existence of an extended narrow line region in PA=12, which coincides with the triplet radio structure (Ulvestad \& Wilson 1984) and the observed outflow of material from the nucleus at PA=10 (Whittle et al. 1988). The ratios of the high to low ionization lines indicate a higher level of gas excitation in PA=12 compared to PA=50. The [NII]6583/H and [SII]6717,31/H versus [OIII]5007/H line ratios are consistent with excitation by an AGN continuum rather than a HII region.
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