The mean ages of S0 disks - Evidence for star formation 5 gigayears ago

Astronomy and Astrophysics – Astronomy

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Galactic Bulge, Galactic Structure, Infrared Astronomy, Spiral Galaxies, Star Formation, Astronomical Photometry, Brightness Distribution, Elliptical Galaxies, Stellar Color

Scientific paper

Optical and infrared photometry of about 35 S0 disks and bulges has been acquired. Comparison to model colors suggests that the disks are 3-5 Gyr younger than the bulges. In some extreme cases, evidence of AGB light is found, indicating that star formation was active as little as 2-3 Gyr ago. This extended period of formation for S0 disks provides the most natural explanation for the prevalence of blue galaxies observed in intermediate redshift clusters of galaxies. The preponderance of S0 galaxies in nearby clusters indicates that they probably were born in that environment and experienced a star formation history that was either terminated by astration or by the process of cluster virialization.

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