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Paper: A Multiwavelength View of Isolated Galaxies
Volume: 480, Structure and Dynamics of Disk Galaxies
Page: 269
Authors: Verdes-Montenegro, L.
Abstract: In the last few years interest in isolated galaxies has been renewed within a context regarding secular evolution. This adds to their value as a control sample for environmental studies of galaxies. This presentation will review important results from recent studies of isolated galaxies. I will emphasize work involving statistically significant samples of isolated galaxies culminating with refinement of the CIG in the AMIGA program. The AMIGA project (Analysis of the interstellar Medium of Isolated Galaxies, has identified a significant sample of the most isolated (Tcc(nearest-neighbor) ∼ 2-3Gyr) galaxies in the local Universe and revealed that they have different properties than galaxies in richer environments. Our analysis of a multiwavelength database includes quantification of degree of isolation, morphologies, as well as FIR and radio line/continuum properties. Properties usually regarded as susceptible to interaction enhancement show lower averages in AMIGA–lower than any galaxy sample yet identified. We find lower MIR/ FIR measures, low levels of radio continuum emission, no radio excess above the radio-FIR correlation, a small number of AGN, and lower molecular gas content. The late-type spiral majority in our sample show very small bulge/total ratios (largely < 0.1) and Sersic indices consistent with an absence of classical bulges. They have redder g–r colors and lower color dispersion for AMIGA subtypes and larger disks, and present the narrowest (Gaussian) distribution of HI profile asymmetries of any sample yet studied.
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