activity
20092018
most citedThe Physics of Crystallization from Globular Cluster White Dwarf Stars in NGC 6397

79 citations · 263 across the 11 of their papers we have counts for

collaborators

10 papers

astro-ph.SR2018★ 8 cited

Outliers: multicolour photometry guiding the search for evolved binary systems in the globular cluster 47 Tucanae

Fabiola Campos, I. Pelisoli, S. Kamann +11

We use Hubble Space Telescope multicolour photometry of the globular cluster 47 Tucanae to uncover a population of 24 objects with no previous classification that are outliers from…

astro-ph.GA2018★ 12 cited

Chemical analysis of eight giant stars of the globular cluster NGC 6366

Arthur A. Puls, Alan Alves-Brito, Fabíola Campos +2

The metal-rich Galactic globular cluster NGC 6366 is the fifth closest to the Sun. Despite its interest, it has received scarce attention, and little is known about its internal st…

astro-ph.SR2016

White Dwarfs in the Metal-Rich Open Cluster NGC 6253

Elizabeth J. Jeffery, Fabiola Campos, Alejandra Romero +1

We have obtained 53 images with the filter and 19 images with the filter, each with 600-second exposures of the super metal rich open cluster NGC 6253 with the Gemini-South…

astro-ph.SR2015★ 35 cited

A comparative analysis of the observed white dwarf cooling sequence from globular clusters

Fabíola Campos, P. Bergeron, A. D. Romero +8

We report our study of features at the observed red end of the white dwarf cooling sequences for three Galactic globular clusters: NGC\,6397, 47\,Tucanae and M\,4. We use deep colo…

astro-ph.SR2015★ 60 cited

The age-metallicity dependence for white dwarfs

A. D. Romero, F. Campos, S. O. Kepler

We present a theoretical study on the metallicity dependence of the initialtofinal mass relation and its influence on white dwarf age determinations. We compute a grid of evo…

astro-ph.SR2015★ 9 cited

Extracting parameters from Colour-Magnitude Diagrams

C. Bonatto, F. Campos, S. O. Kepler +1

We present a simple approach for obtaining robust values of astrophysical parameters from the observed colour-magnitude diagrams (CMDs) of star clusters. The basic inputs are the H…