Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S309(10), p. 73-76, 2014
DOI: 10.1017/s174392131400934x
Full text: Unavailable
AbstractWe have studied the kinematic properties of the ionized gas outflows and ambient interstellar medium (ISM) in a large and representative sample of local U/LIRGs (58 systems, 75 galaxies) at galactic and sub-galactic (i.e.,star-forming clumps) scales, thanks to integral field spectroscopy (IFS)-based high signal-to-noise integrated spectra. The main results have been recently presented in Arribas et al. (2014), and are briefly summarized here.