| Grant number: | 13/18245-0 |
| Support Opportunities: | Scholarships abroad - Research Internship - Post-doctor |
| Start date: | February 01, 2014 |
| End date: | January 31, 2015 |
| Field of knowledge: | Physical Sciences and Mathematics - Astronomy - Stellar Astrophysics |
| Principal Investigator: | Augusto Damineli Neto |
| Grantee: | Leonardo Andrade de Almeida |
| Supervisor: | Hugues Sana |
| Host Institution: | Instituto de Astronomia, Geofísica e Ciências Atmosféricas (IAG). Universidade de São Paulo (USP). São Paulo , SP, Brazil |
| Institution abroad: | Space Telescope Science Institute (STScI), United States |
| Associated to the scholarship: | 12/09716-6 - Accurate distances to young clusters through massive eclipsing binaries, BP.PD |
Abstract 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% (126 binaries). Using a radial velocity monitoring, we will now characterise the orbits of these systems, with the aim of obtaining the first measurements of the period, mass-ratio and eccentricity distributions of massive binaries in a dense and dynamically complex environment, in which conditions are closer to those in super-star-clusters observed beyond the Local Group. We will also constrain the orbital properties of the 18 identified B-supergiant binaries, including an interacting and a post-interaction system. These systems represent key benchmark cases for models of close binary evolution. (AU) | |
| News published in Agência FAPESP Newsletter about the scholarship: | |
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