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Ionized gas outflows and global kinematics of low-z luminous star-forming galaxies

Published online by Cambridge University Press:  09 February 2015

S. Arribas ,
L. Colina ,
E. Bellocchi ,
R. Maiolino  and
M. Villar-Martín
S. Arribas
Affiliation:
CSIC - Departamento de Astrofísica-Centro de Astrobiología (CSIC-INTA), Torrejón de Ardoz, Madrid, Spain email: [email protected]
L. Colina
Affiliation:
CSIC - Departamento de Astrofísica-Centro de Astrobiología (CSIC-INTA), Torrejón de Ardoz, Madrid, Spain email: [email protected]
E. Bellocchi
Affiliation:
CSIC - Departamento de Astrofísica-Centro de Astrobiología (CSIC-INTA), Torrejón de Ardoz, Madrid, Spain email: [email protected]
R. Maiolino
Affiliation:
Cavendish Laboratory, University of Cambridge 19 J. J. Thomson Avenue, Cambridge CB3 0HE, UKand Kavli Institute for Cosmology, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK
M. Villar-Martín
Affiliation:
CSIC - Departamento de Astrofísica-Centro de Astrobiología (CSIC-INTA), Torrejón de Ardoz, Madrid, Spain email: [email protected]
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Abstract

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We 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.

Keywords

- galaxies: evolution - galaxies: ISM -galaxies: Outflows
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Issue S309: Galaxies in 3D across the Universe , July 2014 , pp. 73 - 76
Copyright
Copyright © International Astronomical Union 2015 

References

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