SIMBAD references

2014MNRAS.439.3835D - Mon. Not. R. Astron. Soc., 439, 3835-3846 (2014/April-3)

Starburst-AGN mixing - I. NGC 7130.

DAVIES R.L., RICH J.A., KEWLEY L.J. and DOPITA M.A.

Abstract (from CDS):

We present an integral field spectroscopic study of the luminous infrared galaxy NGC 7130, a known starburst-active galactic nucleus (AGN) composite galaxy. We employ standard emission-line ratio diagnostics and maps of velocity dispersion and velocity field to investigate how the dominant ionizing sources change as a function of radius. From the signatures of both star formation and AGN activity we show that NGC 7130 is a remarkably clean case of starburst-AGN mixing. We find a smooth transition from AGN-dominated emission in the centre to pure star-forming activity further out, from which we can estimate the radius of the extended narrow line region to be 1.8±0.8 kpc. We calculate that the fraction of [Oiii] luminosity due to star formation and AGN activity is 30±2 and 70±3 percent, respectively, and that the fraction of Hα luminosity due to star formation and AGN activity is 65±3 and 35±2 percent, respectively. We conclude with a discussion of the importance and potential of starburst-AGN mixing for future studies of the starburst-AGN connection.

Abstract Copyright: © 2014 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2014)

Journal keyword(s): galaxies: active - galaxies: individual: NGC 7130 - galaxies: Seyfert

Simbad objects: 10

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2021.03.06-00:34:00

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