activity
20172021
most citedOptical/NIR stellar absorption and emission-line indices from luminous infrared galaxies

37 citations · 101 across the 7 of their papers we have counts for

collaborators

12 papers

astro-ph.GA2021

The Puzzling Origin of Massive Compact Galaxies in MaNGA

A. Schnorr-Müller, M. Trevisan, R. Riffel +7

We characterized the kinematics, morphology, and stellar population (SP) properties of a sample of massive compact quiescent galaxies (MCGs, /$M_\odot \le…

astro-ph.GA20206 cited

The properties and environment of very young galaxies in the local Universe

M. Trevisan, G. A. Mamon, T. X. Thuan +3

In the local Universe, there is a handful of dwarf compact star-forming galaxies with extremely low oxygen abundances. It has been proposed that they are young, having formed a lar…

astro-ph.GA202014 cited

Globular Cluster Systems of Relic Galaxies

Karla A. Alamo-Martínez, Ana L. Chies-Santos, Michael A. Beasley +6

We analyse the globular cluster (GC) systems of a sample of 15 massive, compact early-type galaxies (ETGs), 13 of which have already been identified as good relic galaxy candidates…

astro-ph.GA20205 cited

Stellar Population Properties of ETGs in Compact Groups of Galaxies

Tatiana C. Moura, Reinaldo R. de Carvalho, Sandro B. Rembold +6

We present results on the study of the stellar population in Early-Type galaxies (ETGs) belonging to 151 Compact Groups (CGs). We also selected a field sample composed of 846 ETGs…

astro-ph.GA2019

The frequency of very young galaxies in the local Universe: II. The view from SDSS spectra

Gary A. Mamon, Marina Trevisan, Trinh X. Thuan +2

Only a handful of galaxies in the local Universe appear to be very young. We estimate the fraction of very young galaxies (VYGs), defined as those with more than half their stellar…

astro-ph.SR20198 cited

Integrated Spectra of Milky Way Globular Cluster

Tatiana Coelho de Moura, Marina Trevisan, Beatriz Barbuy +1

Integrated spectra of Milky Way globular clusters (GCs) are reproduced by computing synthetic spectra taking into account individual element abundances. Five clusters were selected…