STELLAR POPULATIONS OF BARRED QUIESCENT GALAXIES
STELLAR POPULATIONS OF BARRED QUIESCENT GALAXIES
Selecting centrally quiescent galaxies from the Sloan Digital Sky Survey (SDSS) to create high signal-to-noise ratio ( Å−1) stacked spectra with minimal emission-line contamination, we accurately and precisely model the central stellar populations of barred and unbarred quiescent disk galaxies. By splitting our sample by redshift, we can use the …