170 citations · 170 across the 1 of their papers we have counts for
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Correlations among the properties of galaxies found in a blind HI survey, which also have SDSS optical data
Diego A. Garcia-Appadoo, Andrew A. West, Julianne J. Dalcanton +2
We have used the Parkes Multibeam system and the Sloan Digital Sky Survey (SDSS) to assemble a sample of 195 galaxies selected originally from their HI signature to avoid biases ag…
The UV luminosity function and star formation rate of the Coma cluster
L. Cortese, G. Gavazzi, A. Boselli
We present estimates of the GALEX NUV and FUV luminosity functions (LFs) of the Coma cluster, over a total area of ~9 deg^2 (~25 Mpc^2), i.e. from the cluster center to the virial…
The origin of the mu_e - M_B and Kormendy relations in dwarf elliptical galaxies
A. Boselli, S. Boissier, L. Cortese +1
The present work is aimed at studying the distribution of galaxies of different types and luminosities along different structural scaling relations to see whether massive and dwarf…
Neutral Hydrogen and Star Formation in the Coma-Abell1367 Supercluster
Luca Cortese
We present preliminary results of a multi-wavelength study focused on the evolution of spiral galaxies in the UV-optical colour-magnitude (CM) diagram. By combining HI, UV and opti…
UV Dust Attenuation in Star-forming Galaxies: II Calibrating the A(UV) vs. L_TIR/L_UV relation
L. Cortese, A. Boselli, P. Franzetti +4
We investigate the dependence of the total-infrared (TIR) to UV luminosity ratio method for calculating the UV dust attenuation A(UV) from the age of the underlying stellar populat…
The origin of dwarf ellipticals in the Virgo cluster
A. Boselli, S. Boissier, L. Cortese +1
We study the evolution of dwarf (L_H < 10^{9.6} L_Ho) star forming and quiescent galaxies in the Virgo cluster by comparing their UV to radio centimetric properties to the predicti…