Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: GALÁXIAS, ABUNDÂNCIA ESTELAR
ABNT
BENSBY, T e MORENO, Jorge Luis Meléndez. Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars - VI Age and abundances structure of the stellar populations in the central sub-kpc of the milky way *,**. Astronomy & Astrophysics, v. 605, p. 89, 2017Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201730560. Acesso em: 27 set. 2024.APA
Bensby, T., & Moreno, J. L. M. (2017). Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars - VI Age and abundances structure of the stellar populations in the central sub-kpc of the milky way *,**. Astronomy & Astrophysics, 605, 89. doi:10.1051/0004-6361/201730560NLM
Bensby T, Moreno JLM. Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars - VI Age and abundances structure of the stellar populations in the central sub-kpc of the milky way *,** [Internet]. Astronomy & Astrophysics. 2017 ; 605 89.[citado 2024 set. 27 ] Available from: https://doi.org/10.1051/0004-6361/201730560Vancouver
Bensby T, Moreno JLM. Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars - VI Age and abundances structure of the stellar populations in the central sub-kpc of the milky way *,** [Internet]. Astronomy & Astrophysics. 2017 ; 605 89.[citado 2024 set. 27 ] Available from: https://doi.org/10.1051/0004-6361/201730560