High-resolution abundance analysis of very metal-poor r-I stars (2014)
Fonte: Astronomy & Astrophysics. Unidade: IAG
Assuntos: GALÁXIA (VIA LÁCTEA), GALÁXIAS, ABUNDÂNCIA ESTELAR
ABNT
SIQUEIRA MELLO, C. et al. High-resolution abundance analysis of very metal-poor r-I stars. Astronomy & Astrophysics, v. 565, p. A93/1-A93/23, 2014Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201423826. Acesso em: 31 out. 2024.APA
Siqueira Mello, C., Hill, V., Barbuy, B. L. S., Spite, M., Spite, F., Beers , T. C., et al. (2014). High-resolution abundance analysis of very metal-poor r-I stars. Astronomy & Astrophysics, 565, A93/1-A93/23. doi:10.1051/0004-6361/201423826NLM
Siqueira Mello C, Hill V, Barbuy BLS, Spite M, Spite F, Beers TC, Caffau E, Bonifacio P, Cayrel R, François P, Schatz H, Wanajo S. High-resolution abundance analysis of very metal-poor r-I stars [Internet]. Astronomy & Astrophysics. 2014 ; 565 A93/1-A93/23.[citado 2024 out. 31 ] Available from: https://doi.org/10.1051/0004-6361/201423826Vancouver
Siqueira Mello C, Hill V, Barbuy BLS, Spite M, Spite F, Beers TC, Caffau E, Bonifacio P, Cayrel R, François P, Schatz H, Wanajo S. High-resolution abundance analysis of very metal-poor r-I stars [Internet]. Astronomy & Astrophysics. 2014 ; 565 A93/1-A93/23.[citado 2024 out. 31 ] Available from: https://doi.org/10.1051/0004-6361/201423826