Aims. We compare the predictions of evolutionary models for early-type stars with atmospheric parameters, projected rotational velocities and nitrogen abundances estimated for a sample of Be-type stars. Our targets are located in 4 fields centred on the Large Magellanic Cloud cluster: NGC 2004 and the N 11 region as well as the Small Magellanic Cloud clusters: NGC 330 and NGC 346.
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science
Dunstall, P. R., Brott, I., Dufton, P., Lennon, D. J., Evans, C. J., Smartt, S., & Hunter, I. (2011). The VLT-FLAMES survey of massive stars: Nitrogen abundances for Be-type stars in the Magellanic Clouds. Astronomy and Astrophysics, 536, [A65]. https://doi.org/10.1051/0004-6361/201117588