activity
20042023
most citedSpatial dependence of 2MASS luminosity and mass functions in the old open cluster NGC 188

95 citations · 634 across the 20 of their papers we have counts for

collaborators

20 papers

astro-ph.GA2023★ 21 cited

The VISCACHA survey -- VII. Assembly history of the Magellanic Bridge and SMC Wing from star clusters

R. A. P. Oliveira, F. F. S. Maia, B. Barbuy +15

The formation scenario of the Magellanic Bridge during an encounter between the Large and Small Magellanic Clouds Myr ago, as proposed by -body models, would be impri…

astro-ph.GA2023★ 19 cited

Enlightening the dynamical evolution of Galactic open clusters: an approach using Gaia DR3 and analytical descriptions

M. S. Angelo, J. F. C. Santos, F. F. S. Maia +1

Most stars in our Galaxy form in stellar aggregates, which can become long-lived structures called open clusters (OCs). Along their dynamical evolution, their gradual depletion lea…

astro-ph.SR2022

The VISCACHA survey -- VI. Dimensional study of the structure of 82 star clusters in the Magellanic Clouds

M. Jimena Rodríguez, C. Feinstein, G. Baume +9

We present a study of the internal structure of 82 star clusters located at the outer regions of the Large Magellanic Cloud and the Small Magellanic Cloud using data of the VISCACH…

astro-ph.GA2022★ 8 cited

The VISCACHA survey -- V. Rejuvenating three faint SMC clusters

E. Bica, F. F. S. Maia, R. A. P. Oliveira +9

We present the analysis of three faint clusters of the Small Magellanic Cloud RZ82, HW42 and RZ158. We employed the SOAR telescope instrument SAM with adaptive optics, allowing us…

astro-ph.GA2022★ 39 cited

The VISCACHA survey -- IV. The SMC West Halo in 8D

B. Dias, M. C. Parisi, M. Angelo +18

The structure of the Small Magellanic Cloud (SMC) is very complex, in particular in the periphery that suffers more from the interactions with the Large Magellanic Cloud (LMC). A w…

astro-ph.GA2021★ 20 cited

Investigating Galactic binary cluster candidates with Gaia EDR3

M. S. Angelo, J. F. C. Santos, F. F. S. Maia +1

A number of stellar open cluster (OC) pairs in the Milky Way occupy similar positions in the phase space (coordinates, parallax and proper motions) and therefore may constitute phy…