Carbon to helium ratio the wind of central stars of planetary nebulae with wc spectrum (1992)
- Authors:
- USP affiliated authors: PACHECO, JOSE ANTONIO DE FREITAS - IAG ; COSTA, ROBERTO DELL AGLIO DIAS DA - IAG
- Unidade: IAG
- Subjects: ASTRONOMIA; ASTROFÍSICA ESTELAR; ASTROFÍSICA
- Language: Inglês
- Imprenta:
- Source:
- Título: Proceedings
- Conference titles: International Astronomical Union Symposium. Arochemiry of Cosmic Phenomena
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ABNT
FREITAS PACHECO, José Antonio et al. Carbon to helium ratio the wind of central stars of planetary nebulae with wc spectrum. 1992, Anais.. Dordrecht: Kluwer, 1992. . Acesso em: 10 out. 2024. -
APA
Freitas Pacheco, J. A., Costa, R. D. 'A. D. da, Araujo, F. X., & Petrini, D. (1992). Carbon to helium ratio the wind of central stars of planetary nebulae with wc spectrum. In Proceedings. Dordrecht: Kluwer. -
NLM
Freitas Pacheco JA, Costa RD'AD da, Araujo FX, Petrini D. Carbon to helium ratio the wind of central stars of planetary nebulae with wc spectrum. Proceedings. 1992 ;[citado 2024 out. 10 ] -
Vancouver
Freitas Pacheco JA, Costa RD'AD da, Araujo FX, Petrini D. Carbon to helium ratio the wind of central stars of planetary nebulae with wc spectrum. Proceedings. 1992 ;[citado 2024 out. 10 ] - Helium and oxygen abundances in SMC planetary nebulae
- Abundances in type i planetary nebulae: is the galactic disk presently oxygen deficient
- Nova centauri 1986 - a spectroscopic study
- Abundâncias químicas em estrelas simbióticas
- Júpiter depois do impacto. [Entrevista]
- Chemical composition of nova centauri 1986
- Chemical abundances of symbiotic nebulae . II
- Chemical composition of a southern planetary nebulae sample
- Spectroscopic study of galactic planetary nebulae
- Metallicity indices for multi-population models. II. Bulges of galaxies
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