Are He and N abundances in type I planetary nebulae as high as empirically derived? (1998)
Source: Astrophysical Journal. Unidade: IAG
Assunto: ASTRONOMIA
ABNT
GRUENWALD, Ruth Bomfim e VIEGAS, Sueli Maria Marino. Are He and N abundances in type I planetary nebulae as high as empirically derived?. Astrophysical Journal, v. 501, n. 1, p. 221-227, 1998Tradução . . Acesso em: 20 ago. 2024.APA
Gruenwald, R. B., & Viegas, S. M. M. (1998). Are He and N abundances in type I planetary nebulae as high as empirically derived? Astrophysical Journal, 501( 1), 221-227.NLM
Gruenwald RB, Viegas SMM. Are He and N abundances in type I planetary nebulae as high as empirically derived? Astrophysical Journal. 1998 ; 501( 1): 221-227.[citado 2024 ago. 20 ]Vancouver
Gruenwald RB, Viegas SMM. Are He and N abundances in type I planetary nebulae as high as empirically derived? Astrophysical Journal. 1998 ; 501( 1): 221-227.[citado 2024 ago. 20 ]