The VLT-FLAMES Tarantula Survey

Bibcode
2011BlgAJ..15...29M
Markova, N.; Evans, C. J.; Bastian, N.; Beletsky, Y.; Bestenlehner, J.; Brott, I.; Cantiello, M.; Carraro, G.; Clark, J. S.; Crowther, P. A.; de Koter, A.; de Mink, S. E.; Doran, E.; Dufton, P. L.; Dunstall, P.; Gieles, M.; Gräefener, G.; Henault-Brunet, V.; Herrero, A.; Howarth, I. D.; Langer, N.; Lennon, D. J.; Maíz Appellániz, J.; Najarro, F.; Puls, J.; Sana, H.; Simón-Díaz, S.; Smartt, S. J.; Stroud, V. E.; Taylor, W. D.; van Loon, J. Th.; Vink, J. S.; Walborn, N. R.
Bibliographical reference

Bulgarian Astronomical Journal, Vol. 15, p. 29

Advertised on:
0
2011
Number of authors
33
IAC number of authors
0
Citations
0
Refereed citations
0
Description
The Tarantula survey is an ESO Large Programme which has obtained multi-epochs spectroscopy of over 800 massive stars in the 30 Dor region in the Large Magelanic Cloud. Here we briefly describe the main drivers of the survey and the observational material derived.
Related projects
Projets' image
Physical properties and evolution of Massive Stars
This project aims at the searching, observation and analysis of massive stars in nearby galaxies to provide a solid empirical ground to understand their physical properties as a function of those key parameters that gobern their evolution (i.e. mass, spin, metallicity, mass loss, and binary interaction). Massive stars are central objects to
Sergio
Simón Díaz
In progress
Type
Refereed
Stellar & Interstellar Physics (FEEI)
The Milky Way and the Local Group (MWLG)
Binary stars

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