Fonte: Astronomy & Astrophysics. Unidade: IAG
Assuntos: GALÁXIAS, ESTRELAS, NUVENS DE MAGALHÃES
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ABNT
DIAS, B. et al. Self-consistent physical parameters for five intermediate-age SMC stellar clusters from CMD modelling. Astronomy & Astrophysics, v. 561, p. A106/1-A106/14, 2014Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201322092. Acesso em: 10 ago. 2024.APA
Dias, B., Kerber, L. O., Barbuy, B. L. S., Santiago, B., Ortolani, S., & Balbinot, E. (2014). Self-consistent physical parameters for five intermediate-age SMC stellar clusters from CMD modelling. Astronomy & Astrophysics, 561, A106/1-A106/14. doi:10.1051/0004-6361/201322092NLM
Dias B, Kerber LO, Barbuy BLS, Santiago B, Ortolani S, Balbinot E. Self-consistent physical parameters for five intermediate-age SMC stellar clusters from CMD modelling [Internet]. Astronomy & Astrophysics. 2014 ; 561 A106/1-A106/14.[citado 2024 ago. 10 ] Available from: https://doi.org/10.1051/0004-6361/201322092Vancouver
Dias B, Kerber LO, Barbuy BLS, Santiago B, Ortolani S, Balbinot E. Self-consistent physical parameters for five intermediate-age SMC stellar clusters from CMD modelling [Internet]. Astronomy & Astrophysics. 2014 ; 561 A106/1-A106/14.[citado 2024 ago. 10 ] Available from: https://doi.org/10.1051/0004-6361/201322092
