10 research outputs found
Ultra deep sub-kpc view of nearby massive compact galaxies
Using Gemini North telescope ultra deep and high resolution (sub-kpc) K-band
adaptive optics imaging of a sample of 4 nearby (z~0.15) massive
(~10^{11}M_sun) compact (R<1.5 kpc) galaxies, we have explored the structural
properties of these rare objects with an unprecedented detail. Our surface
brightness profiles expand over 12 magnitudes in range allowing us to explore
the presence of any faint extended envelope on these objects down to stellar
mass densities ~10^{6} M_sun/kpc^{2} at radial distances of ~15 kpc. We find no
evidence for any extended faint tail altering the compactness of these
galaxies. Our objects are elongated, resembling visually S0 galaxies, and have
a central stellar mass density well above the stellar mass densities of objects
with similar stellar mass but normal size in the present universe. If these
massive compact objects will eventually transform into normal size galaxies,
the processes driving this size growth will have to migrate around
2-3x10^{10}M_sun stellar mass from their inner (R<1.7 kpc) region towards their
outskirts. Nearby massive compact galaxies share with high-z compact massive
galaxies not only their stellar mass, size and velocity dispersion but also the
shape of their profiles and the mean age of their stellar populations. This
makes these singular galaxies unique laboratories to explore the early stages
of the formation of massive galaxies.Comment: Accepted for publication in ApJ Letter. Version revised to match the
accepted versio
Early type galaxies have been the predominant morphological class for massive galaxies since only z~1
Present-day massive galaxies are composed mostly of early-type objects. It is
unknown whether this was also the case at higher redshifts. In a hierarchical
assembling scenario the morphological content of the massive population is
expected to change with time from disk-like objects in the early Universe to
spheroid-like galaxies at present. In this paper we have probed this
theoretical expectation by compiling a large sample of massive
(M_{stellar}>10^{11} h_{70}^{-2} M_{Sun}$) galaxies in the redshift interval 0
< z < 3. Our sample of 1082 objects comprises 207 local galaxies selected from
SDSS plus 875 objects observed with the HST belonging to the POWIR/DEEP2 and
GNS surveys. 639 of our objects have spectroscopic redshifts. Our morphological
classification is performed as close as possible to the optical restframe
according to the photometric bands available in our observations both
quantitatively (using the Sersic index as a morphological proxy) and
qualitative (by visual inspection). Using both techniques we find an enormous
change on the dominant morphological class with cosmic time. The fraction of
early-type galaxies among the massive galaxy population has changed from
~20-30% at z~3 to ~70% at z=0. Early type galaxies have been the predominant
morphological class for massive galaxies since only z~1.Comment: 24 pages, 11 figures, 7 tables, MNRAS accepted, acknowledgement adde