Li-rich AGB/RGB stars: abundance correlations with stellar properties (2014)
- Authors:
- USP affiliated authors: MACIEL, WALTER JUNQUEIRA - IAG ; COSTA, ROBERTO DELL' AGLIO DIAS DA - IAG
- Unidade: IAG
- Subjects: ABUNDÂNCIA ESTELAR; ESTRELAS; LÍTIO
- Language: Inglês
- Imprenta:
- Publisher: Universität Wien
- Publisher place: Wien
- Date published: 2014
- Source:
- Conference titles: Why Galaxies Care About AGB Stars
-
ABNT
MACIEL, Walter Junqueira e COSTA, Roberto Dell'Aglio Dias da. Li-rich AGB/RGB stars: abundance correlations with stellar properties. 2014, Anais.. Wien: Universität Wien, 2014. . Acesso em: 14 mar. 2026. -
APA
Maciel, W. J., & Costa, R. D. 'A. D. da. (2014). Li-rich AGB/RGB stars: abundance correlations with stellar properties. In A closer look in space and time: conference programme and abstracts. Wien: Universität Wien. -
NLM
Maciel WJ, Costa RD'AD da. Li-rich AGB/RGB stars: abundance correlations with stellar properties. A closer look in space and time: conference programme and abstracts. 2014 ;[citado 2026 mar. 14 ] -
Vancouver
Maciel WJ, Costa RD'AD da. Li-rich AGB/RGB stars: abundance correlations with stellar properties. A closer look in space and time: conference programme and abstracts. 2014 ;[citado 2026 mar. 14 ] - The time evolution of the Milky Way’s oxygen abundance gradient
- The evolution of the oxygen abundance radial gradient in the Milky Way Galaxy disk
- The role of the Galactic bar in the chemical evolution of the Milky Way
- The evolution of the radial gradient of oxygen abundance in spiral galaxies
- Improving the determination of chemical abundances in planetary nebulae
- Populações estelares do bojo galáctico
- Abundance gradients and star formation in spiral galaxies
- Abundances in photoionized nebulae of the Local Group and nucleosynthesis of intermediate mass stars
- The population of planetary nebulae near the Galactic Centre: chemical abundances
- Planetary nebulae and the bulge-disk interface of the Galaxy
How to cite
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas