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Preprint typeset using L ATEX style emulateapj v. 03/07/07 NEAR-IR INTEGRAL FIELD SPECTROSCOPY STUDY OF THE STAR FORMATION AND AGN OF THE LIRG NGC 5135

By Ro G. Bedregal, Luis Colina, Almudena Alonso-herrero and Santiago Arribas

Abstract

We present a study of the central 2.3 kpc of NGC 5135, a nearby Luminous Infrared Galaxy (LIRG) with an AGN and circumnuclear starburst. Our main results are based on intermediate spectral resolution ( ∼ 3000-4000) near infrared data taken with the SINFONI integral field spectrograph at the ESO VLT. The ionization of the different phases of the interstellar gas and the complex structures of the star formation have been mapped. Individual regions of interest have been identified and studied in detail. For the first time in this galaxy, we have detected the presence of a high excitation ionization cone centered on the AGN by using the [SiVI]λ1.96 µm line. So far, this structure is the largest reported in the literature for this coronal line, extending (in projection) as far as ∼ 600 pc from the galaxy nucleus. In a complex spatial distribution, a variety of mechanisms are driving the gas ionization, including SNe remnant shocks, young stars and AGN photoionization. The excitation of the molecular gas, however, is mainly produced by X-rays and SNe remnant shocks. UV-mechanisms like fluorescence represent a marginal overall contribution to this process, contrary to the expectations we might have for a galaxy with a recent and strong star formation. Our SNe rate estimations from [FeII]λ1.64 µm are in excellen

Year: 2009
OAI identifier: oai:CiteSeerX.psu:10.1.1.315.2857
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