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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Cars for fieldwork and repair of equipments:The itens requested include two Pick-up for fieldwork and funds for maintenance of the da meteorological Tower of IAG.Two Pick-up are needed for fieldwork in Applied Geophysics, in their studies of exploration of mineral resources. Some examples are: silting of rivers and lakes in the Pantanal basin at Mato Grosso (Coxim-MT); studies of arqueol…
The project aims at the participation on the design, construction and scientific use of the MOSAIC spectrograph, to be installed at the Extremely Large Telescope (ELT), the largest optical telescope ever planned, with a mirror of 39m in diameter, being installed in Chile. The excellent quality and future impact in the brazilian astronomical instrumentation and science is at a low cost as …
Summary: The total value of the R.T.I. -FAPESP is BRL 742,375.55. In years prior to R.T.I. <ç<÷FAPESP destined for the IAG was essentially used to provide the Institute with a Center forData Processing (CPD) compatible with your research needs. For such,the CPD of the Department of Astronomy was reformed, which became the Data Centerof IAG, enabling it to absorb new clusters and the more …
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 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)
Chemical abundances in the Galactic bulge are key to understandthe early enrichment from massive supernovae. In particular in the Galactic bulge, the gas was dense and star formation and explosion of the first supernovae caused a fast chemical enrichment. We have a sample of bulge starsobserved at high-resolution spectroscopy with the Very Large Telescope at the European Southern Observat…
(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…
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 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…
(Only some records are available in English at this moment)
Active galactic nuclei (AGNs) occur when a supermassive black hole (SMBH) accretes matter in a considerable rate. Therefore, such objects need the feeding of matter in order to become active. Studies show that there are correlations between the central SMBH and some parameters of their host galaxies, what suggest a co-evolution between galaxies and their central SMBHs. The feeding mechani…
| 3 / 3 | Ongoing research grants |
| 40 / 24 | Completed research grants |
| 6 / 6 | Ongoing scholarships in Brazil |
| 33 / 11 | Completed scholarships in Brazil |
| 9 / 1 | Completed scholarships abroad |
| 91 / 45 | All research grants and scholarships |
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