Published 2004
| Version v1
Conference paper
B stars population in the field of the Large Magellanic Cloud NGC2004: first results with VLT-FLAMES.
Contributors
Others:
- Galaxies, Etoiles, Physique, Instrumentation (GEPI) ; Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris ; Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)
- Institut d'Astrophysique de Paris (IAP) ; Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
- Universite de Valencia Espagne ; Universitat de València (UV)
- Observatoire de la Côte d'Azur (OCA) ; Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
Description
This document presents our very first results on a part of the program: "A study of the Be phenomenon in young open Galactic and Magellanic clusters". It concerns the B stars population in the LMC NGC2004 cluster and its surrounding field observed with the VLT/FLAMES instrumentation with the GIRAFFE spectrograph, at low resolution, in MEDUSA mode. First observational results which concern the ratio $\frac{Be}{B+Be}$ , the nebulosities in the field and the discovery of spectrocopic binaries are presented.
Additional details
Identifiers
- URL
- https://hal.archives-ouvertes.fr/hal-00012549
- URN
- urn:oai:HAL:hal-00012549v1