activity
20052020
most citedOn the Proof of Dark Matter, the Law of Gravity and the Mass of Neutrinos

177 citations · 1.7k across the 35 of their papers we have counts for

collaborators

35 papers

astro-ph.GA2020★ 14 cited

Dynamics of DiskMass Survey galaxies in refracted gravity

Valentina Cesare, Antonaldo Diaferio, Titos Matsakos +1

We test if Refracted Gravity (RG) can describe the dynamics of disk galaxies without resorting to dark matter. RG is a classical theory of gravity where the standard Poisson equati…

astro-ph.GA2016★ 16 cited

The potential role of NGC 205 in generating Andromeda's vast thin co-rotating plane of satellite galaxies

Garry W. Angus, Paul Coppin, Gianfranco Gentile +1

The Andromeda galaxy is observed to have a system of two large dwarf ellipticals and ~13 smaller satellite galaxies that are currently co-rotating in a thin plane, in addition to 2…

astro-ph.GA2015★ 9 cited

Dynamical measurement of the stellar surface density of face-on galaxies

Garry W. Angus, Gianfranco Gentile, Benoit Famaey

The DiskMass survey recently provided measurements of the vertical velocity dispersions of disk stars in a sample of nearly face-on galaxies. By setting the disk scale-heights to b…

astro-ph.GA2015★ 7 cited

Mass models of disk galaxies from the DiskMass Survey in MOND

Garry W. Angus, Gianfranco Gentile, Robert A. Swaters +4

This article explores the agreement between the predictions of Modified Newtonian Dynamics (MOND) and the rotation curves and stellar velocity dispersion profiles measured by the D…

astro-ph.GA2015★ 13 cited

Disk mass and disk heating in the spiral galaxy NGC 3223

G. Gentile, C. Tydtgat, M. Baes +6

We present the stellar and gaseous kinematics of an Sb galaxy, NGC 3223, with the aim of determining the vertical and radial stellar velocity dispersion as a function of radius, wh…

astro-ph.CO2014★ 62 cited

Morphology parameters: substructure identification in X-ray galaxy clusters

Viral Parekh, Kurt van der Heyden, Chiara Ferrari +2

In recent years multi-wavelength observations have shown the presence of substructures related to merging events in a high fraction of galaxy clusters. Clusters can be roughly grou…