to IAU
Symposium 241
Symposium 241
Abstract details
The physical conditions of the ionized gas and the stellar populations in
circumnuclear starbursts
Johan H. Knapen, Marc Sarzi, Lisa M. Mazzuca Abstract
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 characterized by
low-ionization 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 H$\alpha+$N[{\sc ii}] emission lines from DensePak and the
H$\beta$ and [O{\sc iii}] emission from Sauron allow the construction
of diagnostic diagrams that highlight the transition from star
formation in the ring to excitation by high-velocity shocks or by a
central AGN towards the center. DensePak measurements for the [S{\sc
ii}] line ratio reveal very low gas densities in the ring, $N_{\rm
e}~<~100 \,{\rm cm}^{-3}$, characteristic of massive H{\sc ii}
regions. Comparison with MAPPINGS~III models for starbursts with low
gas densities shows that the ring is of roughly solar
metallicity. This suggests that the gas in the circumnuclear ring
originated in a stellar system capable of substantially enriching the
gas metallicity through sustained star formation. 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. We also give a preview of our
results from a similar analysis of the nuclear region of NGC~4314, and
outline the promise of using the techniques developed for other
galaxies.