University of Cambridge > Talks.cam > Kavli Institute for Cosmology Talk Lists > Obesity in the Universe: Why Did Early-Type Galaxies Grow in Size

Obesity in the Universe: Why Did Early-Type Galaxies Grow in Size

Add to your list(s) Download to your calendar using vCal

If you have a question about this talk, please contact Paula younger.

This talk has been canceled/deleted

Once considered the simplest class of galaxy to model and explain, the assembly history of early type galaxies still presents many puzzles. Spectroscopic observations show that the most massive examples completed their star formation earlier than that in their less massive counterparts, in apparent contradiction to popularly-held hierarchical models. Hubble observations have also revealed that many of the most massive early types seen at high redshift are much more compact than their present-day equivalents. This suggests they somehow expanded in size without growing significantly in mass. Clearly, early type galaxies still have a lot to tell us about galaxy formation and assembly. I will reveal the progress being made with new spectroscopic and Hubble data (....but don’t promise to solve all the puzzles).

Refreshments will be available following the seminar.

This talk is part of the Kavli Institute for Cosmology Talk Lists series.

Tell a friend about this talk:

This talk is included in these lists:

This talk is not included in any other list

Note that ex-directory lists are not shown.

 

© 2006-2024 Talks.cam, University of Cambridge. Contact Us | Help and Documentation | Privacy and Publicity