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.
Referencia bibliográfica

Bulgarian Astronomical Journal, Vol. 15, p. 29

Fecha de publicación:
0
2011
Número de autores
33
Número de autores del IAC
0
Número de citas
0
Número de citas referidas
0
Descripción
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.
Proyectos relacionados
Physical properties and evolution of massive stars
Propiedades Físicas y Evolución de Estrellas Masivas
Las estrellas masivas son objetos claves para la Astrofísica. Estas estrellas nacen con más de 8 masas solares, lo que las condena a morir como Supernovas. Durante su rápida evolución liberan, a través de fuertes vientos estelares, gran cantidad de material procesado en su núcleo y, en determinadas fases evolutivas, emiten gran cantidad de
Sergio
Simón Díaz
En ejecución
Tipo
Con árbitro
Estrellas binarias
Física estelar e interestelar (FEEI)
La Vía Láctea y el Grupo Local (MWLG)

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