Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: LENTES GRAVITACIONAIS, CENTRO GALÁCTICO, FORMAÇÃO E EVOLUÇÃO DA GALÁXIA, ABUNDÂNCIA ESTELAR
ABNT
BENSBY, T e MORENO, Jorge Luis Meléndez. Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars V: Evidence for a wide age distribution and a complex MDF. Astronomy & Astrophysics, v. 549, p. A147/1-A147/26, 2013Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201220678. Acesso em: 15 out. 2024.APA
Bensby, T., & Moreno, J. L. M. (2013). Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars V: Evidence for a wide age distribution and a complex MDF. Astronomy & Astrophysics, 549, A147/1-A147/26. doi:10.1051/0004-6361/201220678NLM
Bensby T, Moreno JLM. Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars V: Evidence for a wide age distribution and a complex MDF [Internet]. Astronomy & Astrophysics. 2013 ; 549 A147/1-A147/26.[citado 2024 out. 15 ] Available from: https://doi.org/10.1051/0004-6361/201220678Vancouver
Bensby T, Moreno JLM. Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars V: Evidence for a wide age distribution and a complex MDF [Internet]. Astronomy & Astrophysics. 2013 ; 549 A147/1-A147/26.[citado 2024 out. 15 ] Available from: https://doi.org/10.1051/0004-6361/201220678