Exploring the Structure of Some of the Most Isolated Galaxies in the Local Universe

Mathematics – Logic

Scientific paper

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Scientific paper

The effects of environment on galaxies (i.e. nurture) can be better evaluated if one can compare against the properties of galaxies drawn from a sample of very isolated systems (i.e. nature). A recent morphological reevaluation of the Karachentseva (1973: CIG) sample of isolated galaxies (AMIGA Survey: Verdes-Montenegro et al. 2005; Sulentic et al. 2006) revealed that 63% of the sample were small bulge Sb-Sc spiral galaxies. We examine a subsample of 100 of this core Sb-Sc isolated population (with recession velocities in the range 1500-10000 km/s). Using Sloan Digital Sky Survey (SDSS) i-band images, we perform bulge/disk/bar/AGN decomposition using BUDDA code (de Souza, Gadotti, dos Anjos 2004) . We also derive concentration, assymetry and clumpiness (CAS parameters: Conselice 2003) using g- and i-band images from SDSS. This baseline sample is used to better quantify interaction induced effects in studies that include galaxies selected without an isolation costraint.

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