Infrared Diagnostics We describe the mid- (MIR) and far- (FIR) infrared properties of AMIGA sample. For this aim, we reprocess IRAS MIR/FIR survey data using...

Hα study of a redshift-limited subsample Hα is a good tracer of recent star formation in places where extinction is not high. The aims of...

Star formation in bars As explained in “Hα study of a redshift-limited subsample“, one of the aspects of our project was to study the Hα...

Star formation in outer disks Hierarchical models for galaxy formation as well as N-body/SPH simulations of the evolution of individual disk galaxies, predict an inside-out...

Optical colours of isolated galaxies The optical colors of galaxies reflect their stellar populations and these colors correlate with morphology and environment. The  color-luminosity relation...