activity
19972008
most citedDynamical modelling of luminous and dark matter in 17 Coma early-type galaxies

190 citations · 519 across the 18 of their papers we have counts for

collaborators
Showing 2008 · astro-phShow all

8 papers · 2 filters

astro-ph200869 cited

The High-Mass End of the Black Hole Mass Function: Mass Estimates in Brightest Cluster Galaxies

E. Dalla Bonta', L. Ferrarese, E. M. Corsini +5

We present Hubble Space Telescope imaging and spectroscopic observations of three Brightest Cluster Galaxies, Abell 1836-BCG, Abell 2052-BCG, and Abell 3565-BCG, obtained with the…

astro-ph200836 cited

Early-type galaxies in the near-infrared: 1.5-2.4\mum spectroscopy

M. Cesetti, V. D. Ivanov, L. Morelli +6

Near-infrared (hereafter NIR) data may provide complementary information to the traditional optical population synthesis analysis of unresolved stellar populations because the spec…

astro-ph200871 cited

Stellar Populations of Bulges in 14 Cluster Disc Galaxies

L. Morelli, E. Pompei, A. Pizzella +6

Photometry and long-slit spectroscopy are presented for 14 S0 and spiral galaxies of the Fornax, Eridanus and Pegasus cluster, and NGC 7582 group. The structural parameters of the…

astro-ph200868 cited

Confirmation of a Kinematic Diagnostic for Face-On B/P Bulges

J. Mendez-Abreu, E. M. Corsini, Victor P. Debattista +4

We present the results of high resolution absorption-line spectroscopy of 3 face-on galaxies, NGC 98, NGC 600, and NGC 1703 with the aim of searching for box/peanut (B/P)-shaped bu…

astro-ph200842 cited

Structure and dynamics of galaxies with a low surface brightness disc. I. The stellar and ionised-gas kinematics

A. Pizzella, E. M. Corsini, M. Sarzi +5

(abridged) Photometry and long-slit spectroscopy are presented for a sample of 6 galaxies with a low surface brightness stellar disc and a bulge. The stellar and ionised-gas kinema…

astro-ph2008

The pseudobulge of NGC 1292

L. Morelli, E. Pompei, A. Pizzella +6

The photometric and kinematic properties of Sb NGC 1292 suggest it hosts a pseudobulge. The properties of the stellar population of such a pseudobulge are consistent with a slow bu…