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The extended narrow line region in Mkn79. I.Observations

L. S. Nazarova, P. T. O'Brien, M. J. Ward

astro-pharXiv:astro-ph/9509097

Abstract

We present deep long slit spectra of Mkn79 in position angles PA=12o and PA=50o obtained with the WHT. These data prove the existence of an extended narrow line region in PA=12o, which coincides with the triplet radio structure (Ulvestad \& Wilson 1984) and the observed outflow of material from the nucleus at PA=10o (Whittle et al. 1988). The ratios of the high to low ionization lines indicate a higher level of gas excitation in PA=12o compared to PA=50o. The [NII]λ6583/Hα and [SII]λ6717,31/Hα versus [OIII]λ5007/Hβ line ratios are consistent with excitation by an AGN continuum rather than a HII region.

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