Chemical abundances for 11 bulge stars from high-resolutions, near-IR spectra (2010)
Fonte: Astronomy & Astrophysics. Unidade: IAG
Assuntos: ABUNDÂNCIA ESTELAR, ESTRELAS, INFRAVERMELHO, CENTRO GALÁCTICO, GALÁXIA (VIA LÁCTEA)
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RYDE, N et al. Chemical abundances for 11 bulge stars from high-resolutions, 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: 22 ago. 2024.APA
Ryde, N., Gustafsson, B., Edvardsson, B., Meléndez Moreno, J. L., Alves-Brito, A., Asplund, M., et al. (2010). Chemical abundances for 11 bulge stars from high-resolutions, near-IR spectra. Astronomy & Astrophysics, 509, A20/1-A20/15. doi:10.1051/0004-6361/200912687NLM
Ryde N, Gustafsson B, Edvardsson B, Meléndez Moreno JL, Alves-Brito A, Asplund M, Barbuy BLS, Hill V, Käufl HU, Minniti D, Ortolani S, Renzini A, Zoccali M. Chemical abundances for 11 bulge stars from high-resolutions, near-IR spectra [Internet]. Astronomy & Astrophysics. 2010 ; 509 A20/1-A20/15.[citado 2024 ago. 22 ] Available from: https://doi.org/10.1051/0004-6361/200912687Vancouver
Ryde N, Gustafsson B, Edvardsson B, Meléndez Moreno JL, Alves-Brito A, Asplund M, Barbuy BLS, Hill V, Käufl HU, Minniti D, Ortolani S, Renzini A, Zoccali M. Chemical abundances for 11 bulge stars from high-resolutions, near-IR spectra [Internet]. Astronomy & Astrophysics. 2010 ; 509 A20/1-A20/15.[citado 2024 ago. 22 ] Available from: https://doi.org/10.1051/0004-6361/200912687
