Backlit galaxies by the hundreds: new steps toward the evolution of dust (original) (raw)

Abstract

Photometric analysis of backlit galaxies is a powerful way to measure the extinction in disks, but has hitherto been limited by the number of suitable pairs near enough for analysis. New searches of the SDSS imagery (mostly from the public galaxyzoo.org project) have revealed hundreds of candidate pairs, opening the possibility of tracing extinction properties across Hubble type and surface

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