Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: ESTRELAS, INTERFEROMETRIA, ANÁLISE DE DADOS, SISMOLOGIA
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ABNT
BAZOT, M e MORENO, Jorge Luiz Meléndez. The radius and mass of the close solar twin 18 Scorpii derived from asteroseismology and interferometry. Astronomy & Astrophysics, v. 526, p. L4/1-L4/4, 2011Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201015679. Acesso em: 15 out. 2024.APA
Bazot, M., & Moreno, J. L. M. (2011). The radius and mass of the close solar twin 18 Scorpii derived from asteroseismology and interferometry. Astronomy & Astrophysics, 526, L4/1-L4/4. doi:10.1051/0004-6361/201015679NLM
Bazot M, Moreno JLM. The radius and mass of the close solar twin 18 Scorpii derived from asteroseismology and interferometry [Internet]. Astronomy & Astrophysics. 2011 ; 526 L4/1-L4/4.[citado 2024 out. 15 ] Available from: https://doi.org/10.1051/0004-6361/201015679Vancouver
Bazot M, Moreno JLM. The radius and mass of the close solar twin 18 Scorpii derived from asteroseismology and interferometry [Internet]. Astronomy & Astrophysics. 2011 ; 526 L4/1-L4/4.[citado 2024 out. 15 ] Available from: https://doi.org/10.1051/0004-6361/201015679
