Hiding in plain sight: An abundance of compact massive spheroids in the local Universe
@article{Graham2015HidingIP, title={Hiding in plain sight: An abundance of compact massive spheroids in the local Universe}, author={Alister W. Graham and Bililign T. Dullo and Giulia A. D. Savorgnan}, journal={arXiv: Astrophysics of Galaxies}, year={2015} }
It has been widely remarked that compact, massive, elliptical-like galaxies are abundant at high redshifts but exceedingly rare in the Universe today, implying significant evolution such that their sizes at z ~ 2+/-0.6 have increased by factors of 3 to 6 to become today's massive elliptical galaxies. These claims have been based on studies which measured the half-light radii of galaxies as though they are all single component systems. Here we identify 21 spheroidal stellar systems within 90 Mpc…
57 Citations
DISKY ELLIPTICAL GALAXIES AND THE ALLEGEDLY OVER-MASSIVE BLACK HOLE IN THE COMPACT MASSIVE “ES” GALAXY NGC 1271
- Physics
- 2016
While spiral and lenticular galaxies have large-scale disks extending beyond their bulges, and most local early-type galaxies with 10^{10} < M_*/M_Sun < 2x10^{11} contain a disk (e.g., ATLAS^3D), the…
The Most Massive Galaxies with Large Depleted Cores: Structural Parameter Relations and Black Hole Masses
- PhysicsThe Astrophysical Journal
- 2019
[Abridged] Luminous spheroids (M_V 0.5 kpc are rare and poorly understood. Here we perform detailed decompositions of the composite surface brightness profiles, extracted from archival Hubble Space…
Forming Compact Massive Galaxies
- Physics
- 2015
In this paper we study a key phase in the formation of massive galaxies: the transition of star forming galaxies into massive (M_stars~10^11 Msun), compact (r_e~1 kpc) quiescent galaxies, which takes…
The diverse evolutionary paths of simulated high-z massive, compact galaxies to z = 0
- Physics
- 2016
Massive quiescent galaxies have much smaller physical sizes at high redshift than today. The strong evolution of galaxy size may be caused by progenitor bias, major and minor mergers, adiabatic…
The abundance of compact quiescent galaxies since z ~ 0.6
- Physics
- 2017
We set out to quantify the number density of quiescent massive compact galaxies at intermediate redshifts. We determine structural parameters based on i-band imaging using the Canada–France–Hawaii…
The fate of high-redshift massive compact galaxies
- Physics
- 2016
Massive high-redshift quiescent compact galaxies (nicknamed red nuggets) have been traditionally connected to present-day elliptical galaxies, often overlooking the relationships that they may have…
A normal supermassive black hole in NGC 1277
- Physics
- 2016
The identification of galaxies with `overly massive' black holes requires two measurements: a black hole mass (M_bh) and a host spheroid mass (M_sph,*). Here we provide our measurements for NGC 1277.…
Galaxy And Mass Assembly (GAMA): blue spheroids within 87 Mpc
- Physics
- 2017
In this paper, we test if nearby blue spheroid (BSph) galaxies may become the progenitors of star-forming spiral galaxies or passively evolving elliptical galaxies. Our sample comprises 428 galaxies…
The puzzling origin of massive compact galaxies in MaNGA
- PhysicsMonthly Notices of the Royal Astronomical Society
- 2021
We characterized the kinematics, morphology, and stellar population (SP) properties of a sample of massive compact quiescent galaxies (MCGs, $10\, \lesssim \, \log M_\star$/M$_\odot \, \lesssim \,…
The AIMSS Project III: the stellar populations of compact stellar systems
- Physics
- 2016
In recent years, a growing zoo of compact stellar systems (CSSs) have been found whose physical properties (mass, size, velocity dispersion) place them between classical globular clusters (GCs) and…
References
SHOWING 1-10 OF 277 REFERENCES
The Majority of Compact Massive Galaxies at z~2 are Disk Dominated
- Physics
- 2011
We investigate the stellar structure of massive, quiescent galaxies at z ~ 2, based on Hubble Space Telescope/WFC3 imaging from the Early Release Science program. Our sample of 14 galaxies has…
Strong size evolution of the most massive galaxies since z~2
- Physics
- 2007
Using the combined capabilities of the large near-infrared Palomar/DEEP-2 survey, and the superb resolution of the Advanced Camera for Surveys HST camera, we explore the size evolution of 831 very…
Extremely compact massive galaxies at z ~ 1.4
- Physics
- 2006
The optical rest-frame sizes of 10 of the most massive (∼5 × 10 11 h −2 M� ) galaxies found in the near-infrared MUNICS survey at 1.2 < z < 1.7 are analysed. Sizes are estimated in both the J and…
SUPERDENSE MASSIVE GALAXIES IN THE NEARBY UNIVERSE
- Physics
- 2009
Superdense massive galaxies (re ~ 1 kpc; M ~ 1011 M ☉) were common in the early universe (z 1.5). Within some hierarchical merging scenarios, a non-negligible fraction (1%-10%) of these galaxies is…
Size Evolution of the Most Massive Galaxies at 1.7 < z < 3 from GOODS NICMOS Survey Imaging
- Physics
- 2008
We measure the sizes of 82 massive (M ≥ 1011 M☉) galaxies at 1.7 ≤ z ≤ 3 utilizing deep HST NICMOS data taken in the GOODS North and South fields. Our sample is almost an order of magnitude larger…
On the dearth of compact, massive, red sequence galaxies in the local universe
- Physics
- 2010
We set out to test the claim that the recently identified population of compact, massive, and quiescent galaxies at z ~ 2.3 must undergo significant size evolution to match the properties of galaxies…
MINOR MERGERS AND THE SIZE EVOLUTION OF ELLIPTICAL GALAXIES
- Physics
- 2009
Using a high-resolution hydrodynamical cosmological simulation of the formation of a massive spheroidal galaxy we show that elliptical galaxies can be very compact and massive at high redshift in…
Superdense Galaxies and the Mass-Size Relation at Low Redshift
- Physics
- 2013
We search for massive and compact galaxies (superdense galaxies, hereafter SDGs) at z = 0.03-0.11 in the Padova-Millennium Galaxy and Group Catalogue, a spectroscopically complete sample…
A vast, thin plane of corotating dwarf galaxies orbiting the Andromeda galaxy
- PhysicsNature
- 2013
Radial velocity measurements reveal that the satellites in this structure have the same sense of rotation about their host, and shows conclusively that substantial numbers of dwarf satellite galaxies share the same dynamical orbital properties and direction of angular momentum.
The Assembly of Milky-Way-like Galaxies Since z ~ 2.5
- Physics
- 2013
Galaxies with the mass of the Milky Way dominate the stellar mass density of the universe but it is uncertain how and when they were assembled. Here we study progenitors of these galaxies out to z =…