111 citations · 894 across the 36 of their papers we have counts for
37 papers
Kinematic and stellar population properties of the counter-rotating components in the S0 galaxy NGC 1366
L. Morelli, A. Pizzella, L. Coccato +7
Context. Many disk galaxies host two extended stellar components that rotate in opposite directions. The analysis of the stellar populations of the counter-rotating components prov…
The transformation of Spirals into S0 galaxies in the cluster environment
Mauro D'Onofrio, Paola Marziani, Lucio Buson
We discuss the observational evidences of the morphological transformation of Spirals into S0 galaxies in the cluster environment exploiting two big databases of galaxy clusters: W…
The UV window on counter rotating ETGs: insight from SPH simulations with chemo-photometric implementation
Daniela Bettoni, Paola Mazzei, Roberto Rampazzo +3
The Galaxy Evolution Explorer (GALEX) detected ultraviolet emission in about 50% of multi-spin early-type galaxies (ETGs), suggesting the occurrence of a recent rejuvenation episod…
The UV view of multi spin galaxies: insight from SPH simulations
Daniela Bettoni, Paola Mazzei, Antonina Marino +3
The UV images of GALEX revealed that ~30% of Early Type Galaxies (ETG) show UV emission indicating a rejuvenation episode. In ETGs with multiple spin components this percentage inc…
Spectroscopic evidence of distinct stellar populations in the counter-rotating stellar disks of NGC 3593 and NGC 4550
L. Coccato, L. Morelli, A. Pizzella +3
We present the results of integral-field spectroscopic observations of the two disk galaxies NGC 3593 and NGC 4550 obtained with VIMOS/VLT. Both galaxies are known to host 2 counte…
Galaxy evolution in nearby groups. II. Galaxy evolution in nearby loose groups. II. Photometric and kinematic characterization of USGC U268 and USGC U376 group members in the Leo cloud
A. Marino, H. Plana, R. Rampazzo +8
We present the photometric and kinematic characterization of two groups, USGC U268 and USGC U376 located in different regions of the Leo cloud. U268, composed of 10 catalogued memb…