Source: The Astrofhysical Journal. Unidade: IAG
Subjects: ESTRELAS, ESPECTROMETRIA, FOTOMETRIA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
MIROSHNICHENKO, A.S et al. Toward understanding the B[e] phenomenon: III. Properties of the optical counterpart of IRAS 00470+6429. The Astrofhysical Journal, v. 700, p. 209-220, 2009Tradução . . Acesso em: 08 set. 2024.APA
Miroshnichenko, A. S., Chentsov, E. L., Klochkova, V. G., & Carciofi, A. C. (2009). Toward understanding the B[e] phenomenon: III. Properties of the optical counterpart of IRAS 00470+6429. The Astrofhysical Journal, 700, 209-220.NLM
Miroshnichenko AS, Chentsov EL, Klochkova VG, Carciofi AC. Toward understanding the B[e] phenomenon: III. Properties of the optical counterpart of IRAS 00470+6429. The Astrofhysical Journal. 2009 ; 700 209-220.[citado 2024 set. 08 ]Vancouver
Miroshnichenko AS, Chentsov EL, Klochkova VG, Carciofi AC. Toward understanding the B[e] phenomenon: III. Properties of the optical counterpart of IRAS 00470+6429. The Astrofhysical Journal. 2009 ; 700 209-220.[citado 2024 set. 08 ]
