- Research Grants
bachelor's at Bacharelado em Física from Universidade Estadual de Feira de Santana (2006), master's at Astronomy from Instituto Nacional de Pesquisas Espaciais (2009) and doctorate at Astronomy from Instituto Nacional de Pesquisas Espaciais (2012). Has experience in Astronomy, focusing on Stellar Astrophysics, acting on the following subjects: atividade estelar, flares, manchas, campo magnetico and sol. (Source: Lattes Curriculum)
Confidence in the models of stellar structure and evolution of massive stars depends on the accuracy with which their basic parameters can be measured. The key step consists in determining accurate distances. This parameter is also fundamental for the census of stellar populations in clusters and galaxies. In this context, massive stars are relevant, given their high luminosities. Sever...
A key ingredient missing from current formation and evolution theories of massive stars, and of cluster evolution, is a robust binary fraction and the intrinsic distributions of orbital parameters. The VLT-FLAMES Tarantula Survey (VFTS), which targeted 800 O- and B- stars in 30 Dor, was designed to detect most massive binaries with periods <200 d: the observed O-type binary fraction is ...
(References retrieved automatically from Web of Science and SciELO through information on FAPESP grants and their corresponding numbers as mentioned in the publications by the authors)
|Data from Web of Science|