Polar-ring galaxies: the SDSS view on the symbiotic galaxies
arXiv:1412.2016 · doi:10.1093/mnras/stu2604
Abstract
Polar-ring galaxies are multi-spin systems, showing star formation in a blue late-type component, perpendicular to a red early-type one, revealing how galaxy formation can sometimes occur in successive steps. We perform two-dimensional decomposition in the , , bandpasses of 50 polar-ring galaxies (PRGs) from the Sloan Digital Sky Survey. Each object was fit with a Sérsic host galaxy and a Sérsic ring. Our general results are: (i) The central (host) galaxies of the PRGs are non-dwarf sub- galaxies with colors typical for early-type galaxies. (ii) Polar structures in our sample are, on average, fainter and bluer than their host galaxies. (iii) In most galaxies, the stellar mass M of the polar component is not negligible in comparison with that of the host. (iv) The distributions of the host galaxies on the size -- luminosity and Kormendy diagrams are shifted by to fainter magnitudes in comparison with E/S0 galaxies. It means that the PRGs hosts are more similar to quenched disks than to ordinary early-type galaxies. (v) All the PRGs in our sample are detected in mid-infrared by WISE, and we derive from the 22m luminosity their star formation rate (SFR). Their SFR/M ratio is larger than for the early-type galaxy sample of Atlas, showing that the star forming disk brings a significant contribution to the new stars. Globally, PRGs appear frequently on the green valley in the mass-color diagram, revealing the symbiotic character between a red-sequence host and a blue cloud ring.
arXiv comment8 pages, 11 figures, accepted for publication in MNRAS
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