Abstract
We present preliminary results of our integral field spectroscopy (IFS)
observations to test whether AGN can suppress star formation in
disc-dominated galaxies. We find a lower specific star formation rate
and a different radial Hα profile for AGN than in the control
sample.
| Original language | English |
|---|---|
| Pages (from-to) | 373-373 |
| Journal | Proceedings of the International Astronomical Union |
| Volume | 8 |
| Issue number | S292 |
| DOIs | |
| Publication status | Published - Aug 2012 |
Keywords
- galaxies: active
- HII regions
- galaxies: spiral
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