graduate at Bacharelado Em Física from Instituto de Física da Universidade de São Paulo (1972). , acting on the following subjects: espectroscopia, diagrama cor magnitude, evolucao estelar, aglomerados globulares and sintese de populacoes. (Source: Lattes Curriculum)
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This RTI, in the amount of BRL 567,955.60, corresponds to the IAG portion of variousprojects coordinated by the Institute's professors. Its use was discussed by the set.of professors in the Congregation and in the three Departments and will contemplate the purchaseof servers and storage to enable the virtualization of a significant part of theInstitute's IT services. (AU)
The main aim of this project is to study the stellar populations and structure of the Milky Way, in order to better understand its formation and evolution. The targets are stars of the Galactic Bulge, Halo and Disk. The bulge is studied in terms of the chemical composition of individual stars, as well as kinematics and ages of field and globular cluster stars. The interplay between the ba…
The objective of this proposal is the study of star clusters in the Galactic bulge, and in the Magellanic Clouds, with the aim of better understanding the formation of the bulge, and the interactions between the Clouds and the Milky Way, and as well on the chemical and dynamical evolution of the Magellanic Clouds. We will use data from the Hubble Space Telescope, of exceptional spatial re…
The aim is to work on the writing of the invited review for the Annual Review of Astronomy & Astrophysics, entitled Chemodynamical evolution of the Galactic bulge. The authors are Beatriz Barbuy, Cristina Chiappini and Ortwin Gerhard. These invited reviews are of great importance, and require much dedication, reading papers and interaction among the authors, in order to be able to write a…
(Only some records are available in English at this moment)
Stellar clusters are ubiquitous in all luminous galaxies and can be used as tracers of galaxy formation and evolution if we understand their growth and assembly into their host systems. To this end, issues yet open in our understanding of these objects need to be investigated. Stellar population (SP) models have yet to properly predict properties of globular clusters (GCs) outside our Gal…
In this work we will develop detailed comparisons between the central regions of the milky way galaxy and its morphological twins (SABbc and SBbc). The project of observations of the Milky Way morphological twins will continue, focusing on the study of their nuclei, whose sample was obtained from the data of the Diving3D survey (Deep IFS View of Nuclei of Galaxies). This survey has the go…
The stellar clusters in the Magellanic System are very important for the determination of the star formation history and chemodynamical evolution of these two satellite galaxies. The analysis of their ages and chemical signatures is crucial to distinguish which is the correct model to explain the origin and evolution of the Magellanic Clouds-Milky Way system. There are currently two model…
The Cassegrain U-Band Efficient Spectrograph (CUBES), is the forthcoming ESO VLT spectrograph to be installed at one Cassegrain focus of the VLT with the goal of covering with a high efficiency the UV ground-based region (300 - 400 nm) with intermediate resolution (about 20K).CUBES is a multinational project from ESO partners and Brazil, which is represented here by IAG/USP and LNA/MCTI. …
The galactic bulge is the component of the milky way that is most controversial in terms of its formation process. The aim of this project is the study of globular clusters as tracers of the formation and evolution of the galactic bulge, by means of photometry, spectroscopy, and complemented with dynamical studies. High quality photometry as obtained with the Hubble Space Telescope (HST) …
The study of the Magellanic Clouds and its link with the Milky Way is the aim of this project. We intend to study several questions such as: (i) the impact of tidal forces generated by the interaction between the Magellanic Clouds and the Milky Way, in the dissolution of stellar clusters, (ii) determination of history of star formation and chemical enrichment in the periphery of these ga…
(Only some records are available in English at this moment)
| 2 / 2 | Ongoing research grants |
| 38 / 22 | Completed research grants |
| 3 / 3 | Ongoing scholarships in Brazil |
| 31 / 9 | Completed scholarships in Brazil |
| 8 / 0 | Completed scholarships abroad |
| 82 / 36 | All research grants and scholarships |
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CV Lattes
ORCID