Source: Astrophysical Journal. Unidade: IAG
Subjects: ASTRONOMIA, ASTROFÍSICA ESTELAR
ABNT
SCHIAVON, Ricardo Piorno e BARBUY, Beatriz Leonor Silveira. The temperature scale of metal-rich M giants based on TiO bands: population synthesis in the near-infrared. Astrophysical Journal, v. 510, n. 2 pt.1, p. L934-L943, 1999Tradução . . Acesso em: 18 ago. 2024.APA
Schiavon, R. P., & Barbuy, B. L. S. (1999). The temperature scale of metal-rich M giants based on TiO bands: population synthesis in the near-infrared. Astrophysical Journal, 510( 2 pt.1), L934-L943.NLM
Schiavon RP, Barbuy BLS. The temperature scale of metal-rich M giants based on TiO bands: population synthesis in the near-infrared. Astrophysical Journal. 1999 ; 510( 2 pt.1): L934-L943.[citado 2024 ago. 18 ]Vancouver
Schiavon RP, Barbuy BLS. The temperature scale of metal-rich M giants based on TiO bands: population synthesis in the near-infrared. Astrophysical Journal. 1999 ; 510( 2 pt.1): L934-L943.[citado 2024 ago. 18 ]