Symmetric vs. asymmetric planetary nebulae: morphology and chemical abundances (2011)
- Authors:
- USP affiliated authors: MACIEL, WALTER JUNQUEIRA - IAG ; COSTA, ROBERTO DELL' AGLIO DIAS DA - IAG
- Unidade: IAG
- Subjects: NEBULOSAS; PLANETAS; ABUNDÂNCIAS (ASTRONOMIA)
- Language: Inglês
- Imprenta:
- Publisher: University of Manchester
- Publisher place: Manchester
- Date published: 2011
- Source:
- Título: APN5
- Conference titles: Conference on Asymmetric Planetary Nebulae
-
ABNT
MACIEL, Walter Junqueira e COSTA, Roberto Dell'Aglio Dias da. Symmetric vs. asymmetric planetary nebulae: morphology and chemical abundances. 2011, Anais.. Manchester: University of Manchester, 2011. . Acesso em: 28 out. 2025. -
APA
Maciel, W. J., & Costa, R. D. 'A. D. da. (2011). Symmetric vs. asymmetric planetary nebulae: morphology and chemical abundances. In APN5. Manchester: University of Manchester. -
NLM
Maciel WJ, Costa RD'AD da. Symmetric vs. asymmetric planetary nebulae: morphology and chemical abundances. APN5. 2011 ;[citado 2025 out. 28 ] -
Vancouver
Maciel WJ, Costa RD'AD da. Symmetric vs. asymmetric planetary nebulae: morphology and chemical abundances. APN5. 2011 ;[citado 2025 out. 28 ] - Abundance variations in the galactic disk: planetary nebulae, open clusters and field stars
- Stellar winds from central stars of planetary nebulae: metallicity effects
- The evolution of the Galatic bulge from planetary nebulae
- Metallicity effects on the radiatively driven winds of central stars of planetary nebulae
- Correlações independentes de distância e populações de nebulosas planetárias na galáxia
- Chemical abundances of planetary nebulae in the disk-bulge connection
- Radial gradients and disc formation in spiral galaxies
- Abundâncias de lítio e metalicidade: tendências em estrelas pobres em metais e estrelas AGB/RGB
- Lithium abundances and metallicities: trends from metal-poor and AGB/RGB stars
- Littium abundances and metallicities: trends from metal-poor and AGB/RGB stars
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