Symmetric and asymmetric planetary nebulae and the time variation of the radial abundance gradients (2013)
- Authors:
- USP affiliated authors: MACIEL, WALTER JUNQUEIRA - IAG ; COSTA, ROBERTO DELL' AGLIO DIAS DA - IAG
- Unidade: IAG
- Subjects: PLANETAS; NEBULOSAS; ABUNDÂNCIAS (ASTRONOMIA)
- Language: Inglês
- Imprenta:
- Publisher: Universidad Nacional Autónoma de México
- Publisher place: México
- Date published: 2013
- Conference titles: Asymmetrical Planetary Nebulae Conference
-
ABNT
MACIEL, Walter Junqueira e COSTA, Roberto Dell'Aglio Dias da. Symmetric and asymmetric planetary nebulae and the time variation of the radial abundance gradients. 2013, Anais.. México: Universidad Nacional Autónoma de México, 2013. . Acesso em: 19 mar. 2024. -
APA
Maciel, W. J., & Costa, R. D. 'A. D. da. (2013). Symmetric and asymmetric planetary nebulae and the time variation of the radial abundance gradients. In . México: Universidad Nacional Autónoma de México. -
NLM
Maciel WJ, Costa RD'AD da. Symmetric and asymmetric planetary nebulae and the time variation of the radial abundance gradients. 2013 ;[citado 2024 mar. 19 ] -
Vancouver
Maciel WJ, Costa RD'AD da. Symmetric and asymmetric planetary nebulae and the time variation of the radial abundance gradients. 2013 ;[citado 2024 mar. 19 ] - Parâmetros físicos e abundâncias químicas em nebulosas fotoionizadas extragalácticas: uma amostra de objetos em M96
- Abundâncias químicas de nebulosas planetárias na conexão bojo-disco
- Planetary nebulae as probles of the chemical evolution of the galactic bulge
- Abundance gradients in the galactic disk: space and time variations
- Physical parameters and chemical abundances in bipolar PNe
- Chemical evolution of the Galactic bulge: single and double infall models
- Chemical abundances of newly discovered planetary nebulae in the galactic bulge
- Planetary nebulae and determination of the bulge–disk boundary
- Time variation of radial gradients in the galactic disk: electron temperatures and abundances
- The population of planetary nebulae near the Galactic Centre: chemical abundances
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