VLT/VIMOS integral field spectroscopy of luminous and ultraluminous infrared galaxies: 2D kinematic properties

By E. Bellocchi, S. Arribas, L. Colina, D. Miralles-Caballero. 2013

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Astronomy and Astrophysics 577 (2013): A59 reproduced with permission from Astronomy and Astrophysics

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THE MULTIPHASE STRUCTURE AND POWER SOURCES OF GALACTIC WINDS IN MAJOR MERGERS (2013, background): “Monreal-Ibero et al. (2006, 2010) found a correlation between line ratios and gas velocity dispersion and argued for a tidal origin of merger shocks.”
Ionized gas outflows and global kinematics of low-z luminous star-forming galaxies (2014, background): “Details about the observations, data reduction, and calibration can be found in Monreal-Ibero et al. (2010), RZ11, and Bellocchi et al. (2013).”
THE NATURE OF LINER-LIKE EMISSION IN RED GALAXIES (2011, background): “In a totally different case, in ultraluminous infrared galaxies (ULIRGs), shocks could indeed be responsible for producing the strong LINER-like emission found there (Monreal-Ibero et al. 2006, 2010; Alonso-Herrero et al. 2010).”
GALAXY-WIDE SHOCKS IN LATE-MERGER STAGE LUMINOUS INFRARED GALAXIES (2011, methodology): “Many recent studies across multiple wavelengths are beginning to focus on resolving the detailed ionization structure, kinematics and power sources of local U/LIRGs in order to further our understanding of galaxy evolution both locally and at high redshift.”