First high-precision differential abundance analysis of extremely metal-poor stars (2016)
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, EVOLUÇÃO ESTELAR, POPULAÇÕES ESTELARES, FORMAÇÃO E EVOLUÇÃO DA GALÁXIA
ABNT
REGGIANI, Henrique et al. First high-precision differential abundance analysis of extremely metal-poor stars. Astronomy & Astrophysics, v. 586, p. A67/1-A67/8, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201527439. Acesso em: 04 out. 2024.APA
Reggiani, H., Moreno, J. L. M., Yong, D., Ramírez, I., & Asplund, M. (2016). First high-precision differential abundance analysis of extremely metal-poor stars. Astronomy & Astrophysics, 586, A67/1-A67/8. doi:10.1051/0004-6361/201527439NLM
Reggiani H, Moreno JLM, Yong D, Ramírez I, Asplund M. First high-precision differential abundance analysis of extremely metal-poor stars [Internet]. Astronomy & Astrophysics. 2016 ; 586 A67/1-A67/8.[citado 2024 out. 04 ] Available from: https://doi.org/10.1051/0004-6361/201527439Vancouver
Reggiani H, Moreno JLM, Yong D, Ramírez I, Asplund M. First high-precision differential abundance analysis of extremely metal-poor stars [Internet]. Astronomy & Astrophysics. 2016 ; 586 A67/1-A67/8.[citado 2024 out. 04 ] Available from: https://doi.org/10.1051/0004-6361/201527439