Open AccessNear‐infrared spectra of Seyfert galaxies and line production mechanisms
Author(s) -
Jackson N.,
Beswick R. J.
Publication year - 2007
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1111/j.1365-2966.2007.11467.x
Subject(s) - physics , astrophysics , photoionization , active galactic nucleus , galaxy , radio galaxy , spectral line , astronomy , infrared , luminous infrared galaxy , emission spectrum , line (geometry) , nucleus , ionization , ion , medicine , geometry , mathematics , quantum mechanics , psychiatry
New observations are reported of J ‐band spectra (1.04–1.4 μm) of three Seyfert 2 galaxies, Mkn 34, Mkn 78 and NGC 5929. In each case the spectral range includes the near‐infrared lines of [Fe ii ], [P ii ], He i and Paβ. Each Seyfert galaxy has a known radio jet, and we investigate the infrared line ratios of the nuclear and extended regions of each galaxy compared to the radio structure. In Mkn 34 there is a clear indication of an extranuclear region, probably coincident with a shock induced by the radio jet, in which [Fe ii ] is considerably enhanced, although the nuclear emission is almost certainly the result of photoionization by the continuum of the active nucleus. Similar effects in extranuclear regions are seen in the other objects, in the case of Mkn 78 confirming recent studies by Ramos Almeida et al. A possible detection of extranuclear [P ii ] emission suggests, if real, that photoionization by the active nucleus is the dominant line excitation mechanism over the whole source, including the regions coincident with the radio jet.