Chemical abundances of 11 bulge stars from high-resolution, near-IR spectra (2010)
Fonte: Astronomy & Astrophysics. Unidade: IAG
Assuntos: ABUNDÂNCIA ESTELAR, GALÁXIAS
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ABNT
RYDE, N et al. Chemical abundances of 11 bulge stars from high-resolution, near-IR spectra. Astronomy & Astrophysics, v. 509, p. A20/1-A20/15, 2010Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/200912687. Acesso em: 13 set. 2024.APA
Ryde, N., Meléndez, J., Alves-Brito, A., & Barbuy, B. L. S. (2010). Chemical abundances of 11 bulge stars from high-resolution, near-IR spectra. Astronomy & Astrophysics, 509, A20/1-A20/15. doi:10.1051/0004-6361/200912687NLM
Ryde N, Meléndez J, Alves-Brito A, Barbuy BLS. Chemical abundances of 11 bulge stars from high-resolution, near-IR spectra [Internet]. Astronomy & Astrophysics. 2010 ; 509 A20/1-A20/15.[citado 2024 set. 13 ] Available from: https://doi.org/10.1051/0004-6361/200912687Vancouver
Ryde N, Meléndez J, Alves-Brito A, Barbuy BLS. Chemical abundances of 11 bulge stars from high-resolution, near-IR spectra [Internet]. Astronomy & Astrophysics. 2010 ; 509 A20/1-A20/15.[citado 2024 set. 13 ] Available from: https://doi.org/10.1051/0004-6361/200912687
