CV Lattes
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
bachelor's at Fisica from Universidade de São Paulo (1973), master's at Astronomy from Universidade de São Paulo (1976) and doctorate at Astronomy from Universidade de São Paulo (1988). Full professor at IAG-USP. Has experience in Astronomy, acting on the following subjects: massive stars, eta Carinae, hot stars, infrared photometry and spectroscopy. Author/co-author in 91 papers, 4700 citations (5 n> 100, 1 n>400) index H=39. personal webpage: www.astro.iag.usp.br/~damineli . (Source: Lattes Curriculum)
| Articles published in Pesquisa FAPESP Magazine about the researcher: |
| Alternative route |
| More than an eclipse |
| Más que un mero eclipse |
| Más que un mero eclipse |
| Journey to the stars |
| Rumbo a las estrellas |
| More itemsLess items |
| 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) |
We plan to carry out photometric monitoring of eta Carinae in the period 2025-27 to characterize the "bore hole" phenomenon, which should reach its highest amplitude in the historical series in 2025.7. This is a new phenomenon in Astrophysics that has not yet been adequately characterized either observationally or theoretically. We present a summarized view of the scientific justification…
Astronomy in the 21st century continues to be a vibrant science; the more so as each decade passes. With the new generation of telescopes that is being currently planned, it will be possible to look for habitable Earth-like planets; to the inner regions of circumstellar disks, revealing the mechanisms that drive planetary and stellar formation; to resolve dense stellar populations in the …
The massive binary system Eta Carinae will be passing through periastron on 17 February 2020, when it crosses the meridian around mid-night. This fact and the availability of particular ground-based observing facilities make this the best opportunity ever to monitor the associated spectroscopic and photometric variability. We plan to carry a dense time sampling of its spectrum through the…
High resolution spectroscopy is necessary, among other approaches, to derive chemical abundances from stars in galaxies of the Local Group. The same is valid for galaxy forming clouds projected against background Quasars. Such data enable the study of chemical evolution in neighbor galaxies and at high redshifts. The comparison between galaxies in the local universe with those at high red…
(Only some records are available in English at this moment)
Title: Mechanical design applied to ground-based instrumentation for astronomyThis project aims to train a professional with unique expertise in mechanical engineering for astronomical instrumentation. The areas of activity will be on three possible fronts in different projects. The first is related to MANIFEST (Many-Instrument Fiber System), the robotic fiber optic positioning system tha…
(Only some records are available in English at this moment)
(Only some records are available in English at this moment)
We are proposing a research plan to work with practical and conceptual features of extreme adaptive optics in the MagAO-X and GMagAO-X projects. It is been proposed the collaboration into development and implementation of a reflective Lyot pupil mask, part of a PIAACMC system, for the MagAO-X, and a post-PDR performance assessment of the GMagAO-X. Both projects are led by the Extreme Wave…
We plan to test two scenarios of massive star formation -- disc accretion or coalescence of low mass stars -- from observations of massive young stellar objects (MYSOs). The first step is to identify those high mass objects (M> 8 MSun) that are associated with near-infrared outflows. The second step, consists on the measurement of the parameters of the outflows at their launching points …
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 35…
(Only some records are available in English at this moment)
| 2 / 2 | Ongoing grants |
| 22 / 13 | Completed research grants |
| 4 / 4 | Ongoing scholarships in Brazil |
| 21 / 13 | Completed scholarships in Brazil |
| 9 / 7 | Completed scholarships abroad |
| 58 / 39 | All research grants and scholarships |
| Associated processes | |