Dynamical masses of early-type galaxies at z~2: Are they truly superdense?

Details Dynamical masses of early-type galaxies at z~2: Are they truly superdense? Dynamical masses of early-type galaxies at z~2: Are they truly superdense?

2009-06-19

arxiv.org/abs/0906.3648v2

Astrophys.J.704:L34-L39,2009

Astronomy and Astrophysics

Astrophysics

Galaxy Astrophysics

6 pages, 4 figures, LaTeX with emulateapj. Accepted for publication in ApJ Letters

Scientific paper

10.1088/0004-637X/704/1/L34

We measured stellar velocity dispersions sigma and dynamical masses of 9 massive (M~10^11 Msun) early-type galaxies (ETG) from the GMASS sample at redshift 1.4

Affiliated with

Also associated with

No associations

Rating

Dynamical masses of early-type galaxies at z~2: Are they truly superdense? does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Dynamical masses of early-type galaxies at z~2: Are they truly superdense?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dynamical masses of early-type galaxies at z~2: Are they truly superdense? will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-401611