CV Lattes
ResearcherID
ORCID
Google Scholar Citations
Universidade de São Paulo (USP). Instituto de Astronomia, Geofísica e Ciências Atmosféricas (IAG) (Institutional affiliation from the last research proposal) Birthplace: Brazil
Carlos Eduardo Barbosa in research grants and scholarships supported by FAPESP.
| News published in Agência FAPESP Newsletter about the researcher |
| More itemsLess items |
| TITULO |
| Articles published in other media outlets ( ): |
| More itemsLess items |
| VEICULO: TITULO (DATA) |
| VEICULO: TITULO (DATA) |
Despite the great efforts and progress made in the last decades, there are still many open questions in the field of galaxy evolution. Two of them are: what are the physical mechanisms responsible for the star formation quenching? In which environment morphological transformations happen? The answer to these questions require the detailed observation of the stellar populations and kinemat…
Although one of the most common environments in the universe, groups of galaxies have been relatively little studied. The majority of papers devoted to understand the role of the environment on the galactic properties made use of the rare and extreme environment of galaxy clusters. However, the group environment can give us the best informations about the galaxy evolution and the physical…
We plan to investigate how well the luminous matter traces the dark matter component of galaxies by studying a sample of 200 nearby field spiral galaxies for which velocity maps and R band images are available. A quarter of the photometric data for this project has already been reduced and calibrated by the student and the velocity fields are available in the literature. The whole projec…
The Initial Mass Function (IMF) is a fundamental aspect of galaxies, yet its determination in galaxies other than the Milky Way has shown conflicting results among studies in the literature. Some works in the last decade have indicated that the IMF is bottom-heavy in relation to the Milky Way, indicating that dwarf stars in those systems are more common than in our own Galaxy, but the sam…
One of the major topics in Astronomy is the role of the environment on galactic properties, mainly due to our poor understanding of the physical mechanisms that act on the baryonic gas of galaxies. In this project, we plan to shed light on the subject by studying the core of the galaxy cluster Hydra I, combining deep photometry from VLT/FORS1 with high signal-to-noise multi-slit spectra f…
| 3 / 3 | Completed scholarships in Brazil |
| 2 / 2 | Completed scholarships abroad |
| 5 / 5 | All Scholarships |
| Associated processes | |