Oxygen abundances in the large magellanic cloud: a prediction of 'SN'ii / 'SN'i rates (1994)
Source: Astronomy and Astrophysics. Unidade: IAG
Subjects: ASTRONOMIA, ASTROFÍSICA ESTELAR, ASTROFÍSICA ESTELAR
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BARBUY, Beatriz Leonor Silveira e FREITAS PACHECO, José Antonio e CASTRO, S. Oxygen abundances in the large magellanic cloud: a prediction of 'SN'ii / 'SN'i rates. Astronomy and Astrophysics, v. 283, n. 1, p. 32-36, 1994Tradução . . Acesso em: 07 nov. 2024.APA
Barbuy, B. L. S., Freitas Pacheco, J. A., & Castro, S. (1994). Oxygen abundances in the large magellanic cloud: a prediction of 'SN'ii / 'SN'i rates. Astronomy and Astrophysics, 283( 1), 32-36.NLM
Barbuy BLS, Freitas Pacheco JA, Castro S. Oxygen abundances in the large magellanic cloud: a prediction of 'SN'ii / 'SN'i rates. Astronomy and Astrophysics. 1994 ; 283( 1): 32-36.[citado 2024 nov. 07 ]Vancouver
Barbuy BLS, Freitas Pacheco JA, Castro S. Oxygen abundances in the large magellanic cloud: a prediction of 'SN'ii / 'SN'i rates. Astronomy and Astrophysics. 1994 ; 283( 1): 32-36.[citado 2024 nov. 07 ]
