Munich Joint Astronomy Colloquium: The Evolution of the Galaxy Mass-Size Relation in Different Environments
by
Simona Mei(JHU)
→
Europe/Berlin
Auditorium (Eso, Garching)
Auditorium
Eso, Garching
Description
We present our recent results on the evolution of the galaxy mass-size relation in different environments up to z~1.3. We find that results on the evolution of the mass-size relation depend on how galaxies are morphologically selected (visually or by their sersic indices). When we select early-type galaxies (ETG) by visual morphology, the field mass-size relation does not show significant evolution from z~1.3 to the present in the mass range we probe. Interestingly, this is in contrast from what is observed at higher masses. In denser environments, the ETG mass-size relation at z~1.3 is shifted towards smaller sizes.