Computer Science
Scientific paper
Feb 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009noao.prop..277r&link_type=abstract
NOAO Proposal ID #2009A-0277
Computer Science
Scientific paper
We have selected early-type galaxies with extremely high velocity dispersions (σ~eq 400 km s^-1) from the SDSS and studied their morphology with the HST-ACS. We now propose to use GMOS to study the kinematics of 8 of the highest-σ galaxies, including 6 which are elongated and extremely compact and dense, and (we believe) may be rapidly rotating. Deep long-slit spectra will provide rotation curves.
Bernardi Mariangela
Hyde Joseph
Roche Nathan
No associations
LandOfFree
Kinematics of extremely high velocity dispersion E/S0 galaxies in the SDSS 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 Kinematics of extremely high velocity dispersion E/S0 galaxies in the SDSS, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Kinematics of extremely high velocity dispersion E/S0 galaxies in the SDSS will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1244773