Abundance gradients: tracing the chemical properties of the disk (2010)
- Authors:
- USP affiliated authors: COSTA, ROBERTO DELL' AGLIO DIAS DA - IAG ; MACIEL, WALTER JUNQUEIRA - IAG
- Unidade: IAG
- Subjects: GALÁXIAS; ABUNDÂNCIAS (ASTRONOMIA)
- Language: Inglês
- Imprenta:
- Publisher: Cambridge University Press
- Publisher place: Cambridge
- Date published: 2010
- ISBN: 9781107005334
- Source:
- Título do periódico: IAU Highlights of Astronomy, v.15
- Conference titles: IAU General Assembly
-
ABNT
COSTA, Roberto Dell'Aglio Dias da e MACIEL, Walter Junqueira. Abundance gradients: tracing the chemical properties of the disk. 2010, Anais.. Cambridge: Cambridge University Press, 2010. . Acesso em: 25 abr. 2024. -
APA
Costa, R. D. 'A. D. da, & Maciel, W. J. (2010). Abundance gradients: tracing the chemical properties of the disk. In IAU Highlights of Astronomy, v.15. Cambridge: Cambridge University Press. -
NLM
Costa RD'AD da, Maciel WJ. Abundance gradients: tracing the chemical properties of the disk. IAU Highlights of Astronomy, v.15. 2010 ;[citado 2024 abr. 25 ] -
Vancouver
Costa RD'AD da, Maciel WJ. Abundance gradients: tracing the chemical properties of the disk. IAU Highlights of Astronomy, v.15. 2010 ;[citado 2024 abr. 25 ] - 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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