University of Cambridge > Talks.cam > Cavendish Astrophysics Seminars > Galaxy Bimodality and Post-Starburst Galaxies

Galaxy Bimodality and Post-Starburst Galaxies

Download to your calendar using vCal

If you have a question about this talk, please contact Greg Willatt .

Post-starburst galaxies have long been known as an intriguing class of galaxies, identified through their unusual optical spectra as having had a recent burst of star formation that has since quenched. What cause the starburst and what caused the quenching? Originally identified in clusters (so-called E+A or K+A galaxies), they are now known to exist in all environments. They are rare at low-redshift, but increasingly common at high redshift. I will review recent progress in studying post-starburst galaxy properties, focussing on the question of whether they are true โ€˜transitionโ€™ species, i.e. galaxies transiting from the blue cloud to the red sequence, and how important they could be for accounting for the growth of the red sequence since z~2.

This talk is part of the Cavendish Astrophysics Seminars series.

This talk is included in these lists:

Note that ex-directory lists are not shown.

 

ยฉ 2006-2025 Talks.cam, University of Cambridge. Contact Us | Help and Documentation | Privacy and Publicity