Chemical evolution of the Magellanic Clouds based on planetary nebulae (2008)
- Authors:
- USP affiliated authors: MACIEL, WALTER JUNQUEIRA - IAG ; COSTA, ROBERTO DELL' AGLIO DIAS DA - IAG ; IDIART, THAIS EUNICE PIRES - IAG
- Unidade: IAG
- Subjects: NUVENS DE MAGALHÃES; ABUNDÂNCIAS (ASTRONOMIA); FORMAÇÃO E EVOLUÇÃO DA GALÁXIA; GALÁXIA (VIA LÁCTEA)
- Language: Inglês
- Imprenta:
- Publisher: International Astronomical Union
- Publisher place: Paris
- Date published: 2008
- Source:
- Conference titles: IAU Symposium
-
ABNT
MACIEL, Walter Junqueira e COSTA, Roberto Dell'Aglio Dias da e IDIART, Thais Eunice Pires. Chemical evolution of the Magellanic Clouds based on planetary nebulae. 2008, Anais.. Paris: International Astronomical Union, 2008. . Acesso em: 24 jan. 2026. -
APA
Maciel, W. J., Costa, R. D. 'A. D. da, & Idiart, T. E. P. (2008). Chemical evolution of the Magellanic Clouds based on planetary nebulae. In The Magellanic System : stars, gas, and galaxies : proceedings. Paris: International Astronomical Union. -
NLM
Maciel WJ, Costa RD'AD da, Idiart TEP. Chemical evolution of the Magellanic Clouds based on planetary nebulae. The Magellanic System : stars, gas, and galaxies : proceedings. 2008 ;[citado 2026 jan. 24 ] -
Vancouver
Maciel WJ, Costa RD'AD da, Idiart TEP. Chemical evolution of the Magellanic Clouds based on planetary nebulae. The Magellanic System : stars, gas, and galaxies : proceedings. 2008 ;[citado 2026 jan. 24 ] - Helium abundances in planetary nebulae: nucleosynthesis and chemical evolution
- Ages of central stars of planetary nebulae
- Planetary nebulae and the chemical evolution of the Magellanic Clouds
- Primordial helium abundance of the SMC: a view from intermediate mass stars
- Chemical composition of planetary nebulae: the galaxy and the magellanic clouds
- Composição química de nubulosas planetárias da galáxia e das nuvens de magalhães
- Stellar populations in the local group: contribution from planetary nebulae
- Age distribution of AGB stars and central stars planetary nebulae
- Metallicity effects on the modified wind momentum of CSPN
- Age distribution of the central stars of galactic disk planetary nebulae
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