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20022026
most citedSuperdense Massive Galaxies in Wings Local Clusters

170 citations · 1.5k across the 40 of their papers we have counts for

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6 papers · 1 filter

astro-ph2008★ 14 cited

The bright galaxy population of five medium redshift clusters. I. Color-Magnitude Relation, Blue Fractions and Visual Morphology

B. Ascaso, M. Moles, J. A. L. Aguerri +2

Using data of five clusters of galaxies within the redshift range 0.15 z 0.25, imaged with the Nordic Optical Telescope (NOT) in the central 1 Mpc in ve…

astro-ph2007★ 94 cited

A spectrophotometric model applied to cluster galaxies: the WINGS dataset

J. Fritz, B. M. Poggianti, D. Bettoni +8

[Abridged] The WIde-field Nearby Galaxy-cluster Survey (WINGS) is a project aiming at the study of the galaxy populations in clusters in the local universe (0.04<z<0.07) and the in…

astro-ph2007★ 83 cited

Substructures in WINGS clusters

M. Ramella, A. Biviano, A. Pisani +10

We search for and characterize substructures in the projected distribution of galaxies observed in the wide field CCD images of the 77 nearby clusters of the WIde-field Nearby Gala…

astro-ph2004★ 8 cited

The peculiar galaxy IC 1182: An ongoing merger?

M. Moles, D. Bettoni, G. Fasano +2

Broad and narrow band images and long slit spectroscopy of IC1182 are presented. The broad band images reveal a distorted morphology with a large, heavily obscured disk-like struct…

astro-ph2003★ 25 cited

Long slit spectroscopy of a sample of isolated spirals with and without an AGN

I. Marquez, F. Durret, J. Masegosa +6

We present the kinematical data obtained for a sample of active (Seyfert) and non active isolated spiral galaxies, based on long slit spectra along several position angles in the H…

astro-ph2002★ 58 cited

Rotation curves and metallicity gradients from HII regions in spiral galaxies

I. Marquez, J. Masegosa, M. Moles +3

In this paper we study long slit spectra in the region of H emission line of a sample of 111 spiral galaxies with recognizable and well defined spiral morphology and with a well…