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Physical conditions of ionized gas and stellar populations in circumnuclear starbursts

Published online by Cambridge University Press:  01 December 2006

Johan H. Knapen ,
Lisa M. Mazzuca  and
Marc Sarzi
Johan H. Knapen
Affiliation:
Instituto de Astrofísica de Canarias, E-38200 La Laguna, Spain University of Hertfordshire, Hatfield, AL10 9AB, UK
Lisa M. Mazzuca
Affiliation:
NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
Marc Sarzi
Affiliation:
University of Hertfordshire, Hatfield, AL10 9AB, UK
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Abstract

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We present an emission-line diagnostic analysis of integral-field spectroscopic observations that cover the circumnuclear ring-like regions in a small number of spiral galaxies. We concentrate on the specific case of the Sa galaxy NGC 7742, which hosts a spectacular circumnuclear starburst ring and nuclear regions characterised by low-ionisation emission. The gas in the ring rotates in the opposite sense to the stars in the galaxy, suggesting a recent merging or acquisition event. The combination of integral-field measurements for the Hα+N[ii] emission lines from DensePak and the Hβ and [Oiii] emission from SAURON allows the construction of diagnostic diagrams that highlight the transition from star formation in the ring to excitation by high-velocity shocks or by an AGN near the centre. DensePak measurements for the [Sii] line ratio reveal very low gas densities in the ring, Ne<100 cm−3, characteristic of massive Hii regions. Comparison with MAPPINGS III models for starbursts with low gas densities shows that the ring is of roughly solar metallicity. We suggest that NGC 7742 cannibalised a smaller galaxy rich in metal-poor gas, and that star formation episodes in the ring have since increased the metallicity to its present value.

Keywords

galaxies: evolutiongalaxies: individual (NGC 7742)galaxies: ISMgalaxies: kinematics and dynamicsgalaxies: nucleigalaxies: spiralgalaxies: starburst
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S241: Stellar Populations as Building Blocks of Galaxies , December 2006 , pp. 517 - 518
Copyright
Copyright © International Astronomical Union 2007

References

Allard, E. L., Sarzi, M., Knapen, J. H. & Mazzuca, L. M. 2007, MNRAS, submittedGoogle Scholar
Falcón-Barroso, J. & the SAURON team 2006, MNRAS 369, 259Google Scholar
Kewley, L. J., Dopita, M. A., Sutherland, R. S., Heisler, C. A. & Trevena, J. 2001, ApJ 556, 121CrossRefGoogle Scholar
Knapen, J. H. 2005, A&A 429, 141Google Scholar
Knapen, J. H., Beckman, J. E., Heller, C. H., Shlosman, I. & de Jong, R. S. 1995, ApJ 454, 623Google Scholar
Mazzuca, L. M., Sarzi, M., Knapen, J. H., Veilleux, S. & Swaters, R. 2006, ApJ 649, L77Google Scholar
de Zeeuw, T. & the SAURON team 2002, MNRAS 329, 513CrossRefGoogle Scholar