102 citations · 176 across the 5 of their papers we have counts for
6 papers
ALMA detection of the dusty object silhouetted against the S0 galaxy NGC 3269 in the Antlia cluster
L. K. Haikala, R. Salinas, T. Richtler +3
An intriguing silhouette of a small dust patch can be seen against the disk of the S0 galaxy NGC 3269 in the Antlia cluster in optical images. The images do not provide any clue as…
Evidence of a fast bar in the weakly-interacting galaxy NGC 4264 with MUSE
V. Cuomo, E. M. Corsini, J. A. L. Aguerri +9
We present surface photometry and stellar kinematics of NGC 4264, a barred lenticular galaxy in the region of the Virgo Cluster undergoing a tidal interaction with one of its neigh…
The Fornax 3D project: Thick disks in a cluster environment
F. Pinna, J. Falcón-Barroso, M. Martig +13
We used deep MUSE observations to perform a stellar-kinematic and population analysis of FCC 153 and FCC 177, two edge-on S0 galaxies in the Fornax cluster. The geometrical definit…
The Fornax 3D project: unveiling the thick disk origin in FCC 170: signs of accretion?
F. Pinna, J. Falcón-Barroso, M. Martig +13
We present and discuss the stellar kinematics and populations of the S0 galaxy FCC 170 (NGC 1381) in the Fornax cluster, using deep MUSE data from the Fornax 3D survey. We show the…
Radial trends in Galactic globular clusters and their possible origin
Valery V. Kravtsov
The relaxation time at the half-mass radius of Galactic globular clusters (GGCs) is typically within a few Gyr. Hence, the majority of GGCs are expected to be well relaxed systems,…
Fossil group origins IX. Probing the formation of fossil galaxy groups with stellar population gradients of their central galaxies
E. M. Corsini, L. Morelli, S. Zarattini +7
Fossil groups (FGs) are galaxy aggregates with an extended and luminous X-ray halo, which are dominated by a very massive early-type galaxy and lack of L* objects. FGs are indeed c…