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Galaxy and Mass Assembly (GAMA): Accurate number densities and environments of massive ultra-compact galaxies at 0.02 < z < 0.3

Buitrago, F.; Ferreras, I.; Kelvin, L. S.; Baldry, I. K.; Davies, L.; Angthopo, J.; Khochfar, S.; Hopkins, A. M.; Driver, S. P.; Brough, S.; Sabater, J.; Conselice, C. J.; Liske, J.; Holwerda, B. W.; Bremer, M. N.; Phillipps, S.; López-Sánchez, Á. R.; Graham, A. W.

Galaxy and Mass Assembly (GAMA): Accurate number densities and environments of massive ultra-compact galaxies at 0.02 < z < 0.3 Thumbnail


F. Buitrago

I. Ferreras

L. S. Kelvin

I. K. Baldry

L. Davies

J. Angthopo

S. Khochfar

A. M. Hopkins

S. P. Driver

S. Brough

J. Sabater

C. J. Conselice

J. Liske

B. W. Holwerda

M. N. Bremer

S. Phillipps

Á. R. López-Sánchez

A. W. Graham


Context. Massive ultra-compact galaxies (MUGs) are common at z = 2−3, but very rare in the nearby Universe. Simulations predict that the few surviving MUGs should reside in galaxy clusters, whose large relative velocities prevent them from merging, thus maintaining their original properties (namely stellar populations, masses, sizes and dynamical state).

Aims. Our goal is to obtain a complete census of the MUG population at 0.02 < z < 0.3, determining the number density, population properties and environment.

Methods. We have taken advantage of the high-completeness, large-area spectroscopic GAMA survey, complementing it with deeper imaging from the KiDS and VIKING surveys. We find a set of 22 bona-fide MUGs, defined as having high stellar mass (> 8 × 1010 M⊙) and compact size (Re < 2 kpc). An additional set of seven lower-mass objects (6 × 1010 < M⋆/M⊙ < 8 × 1010) are also potential candidates according to typical mass uncertainties.

Results. The comoving number density of MUGs at low redshift (z < 0.3) is constrained at (1.0 ± 0.4)×10−6 Mpc−3, consistent with galaxy evolution models. However, we find a mixed distribution of old and young galaxies, with a quarter of the sample representing (old) relics. MUGs have a predominantly early or swollen disk morphology (Sérsic index 1 < n < 2.5) with high stellar surface densities (⟨Σe⟩∼1010 M⊙ Kpc−2). Interestingly, a large fraction feature close companions – at least in projection – suggesting that many (but not all) reside in the central regions of groups. Halo masses show these galaxies inhabit average-mass groups.

Conclusions. As MUGs are found to be almost equally distributed among environments of different masses, their relative fraction is higher in more massive overdensities, matching the expectations that some of these galaxies fell in these regions at early times. However, there must be another channel leading some of these galaxies to an abnormally low merger history because our sample shows a number of objects that do not inhabit particularly dense environments.


Buitrago, F., Ferreras, I., Kelvin, L. S., Baldry, I. K., Davies, L., Angthopo, J., …Graham, A. W. (2018). Galaxy and Mass Assembly (GAMA): Accurate number densities and environments of massive ultra-compact galaxies at 0.02 < z < 0.3. Astronomy and Astrophysics, 619, Article A137.

Journal Article Type Article
Acceptance Date Sep 3, 2018
Online Publication Date Nov 16, 2018
Publication Date 2018-11
Deposit Date Dec 3, 2018
Publicly Available Date Dec 3, 2018
Journal Astronomy & Astrophysics
Electronic ISSN 1432-0746
Publisher EDP Open
Peer Reviewed Peer Reviewed
Volume 619
Article Number A137
Keywords Space and Planetary Science; Astronomy and Astrophysics
Public URL
Publisher URL


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Copyright Statement
Reproduced with permission from Astronomy & Astrophysics, © ESO

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