activity
20072024
most citedA comprehensive picture of baryons in groups and clusters of galaxies

90 citations · 454 across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.HE2024★ 2 cited

Orbital motion of NGC 6166 (3C 338) and its impact on the jet morphology at kiloparsec scales

A. S. R. Antas, A. Caproni, R. E. G. Machado +2

In the central region of the galaxy cluster Abell 2199 (A2199) resides the cD galaxy NGC 6166, which spatially coincides with the 3C 338 radio source. Lobes, jets, and a more detac…

astro-ph.GA2023★ 12 cited

The effect of cluster dynamical state on ram-pressure stripping

A. C. C. Lourenço, Y. L. Jaffé, B. Vulcani +14

Theoretical and observational studies have suggested that ram-pressure stripping by the intracluster medium can be enhanced during cluster interactions, boosting the formation of t…

astro-ph.CO2019★ 31 cited

Physical properties of the X-ray gas as a dynamical diagnosis for galaxy clusters

T. F. Laganá, F. Durret, P. A. A. Lopes

We analysed XMM-{\it Newton} EPIC data for 53 galaxy clusters. Through 2D spectral maps, we provide the most detailed and extended view of the spatial distribution of temperature (…

astro-ph.GA2018★ 14 cited

Star-formation rates of cluster galaxies: nature vs nurture

Tatiana F. Lagana, M. P. ulmer

We analyzed 17 galaxy clusters, and investigated, for the first time, the dependence of the SFR and sSFR as a function of projected distance (as a proxy for environment) and stella…

astro-ph.CO2014

Structure in galaxy clusters

Gastao B. Lima Neto, Tatiana F. Lagana, Felipe Andrade-Santos +1

We will discuss here how structures observed in clusters of galaxies can provide us insight on the formation and evolution of these objects. We will focus primarily on X-ray observ…

astro-ph.CO2013★ 90 cited

A comprehensive picture of baryons in groups and clusters of galaxies

T. F. Lagana, N. Martinet, F. Durret +3

(Abridged) Based on XMM-Newton, Chandra and SDSS data, we investigate the baryon distribution in groups and clusters and its use as a cosmological constraint. For this, we consider…