Improving the determination of chemical abundances in planetary nebulae (2017)
- Authors:
- USP affiliated authors: MACIEL, WALTER JUNQUEIRA - IAG ; COSTA, ROBERTO DELL'AGLIO DIAS DA - IAG
- Unidade: IAG
- Assunto: NEBULOSAS
- Language: Inglês
- Imprenta:
- Publisher: Cornell University
- Publisher place: Ithaca, N.Y.
- Date published: 2017
- Source:
- Título: ARXIV
- Conference titles: Workshop Chemical Abundances in Gaseous Nebulae
-
ABNT
CAVICHIA, O et al. Improving the determination of chemical abundances in planetary nebulae. 2017, Anais.. Ithaca, N.Y.: Cornell University, 2017. Disponível em: https://arxiv.org/pdf/1612.03672.pdf. Acesso em: 04 mar. 2026. -
APA
Cavichia, O., Costa, R. D. 'A. D. da, Maciel, W. J., & Mollá, M. (2017). Improving the determination of chemical abundances in planetary nebulae. In ARXIV. Ithaca, N.Y.: Cornell University. Recuperado de https://arxiv.org/pdf/1612.03672.pdf -
NLM
Cavichia O, Costa RD'AD da, Maciel WJ, Mollá M. Improving the determination of chemical abundances in planetary nebulae [Internet]. ARXIV. 2017 ;[citado 2026 mar. 04 ] Available from: https://arxiv.org/pdf/1612.03672.pdf -
Vancouver
Cavichia O, Costa RD'AD da, Maciel WJ, Mollá M. Improving the determination of chemical abundances in planetary nebulae [Internet]. ARXIV. 2017 ;[citado 2026 mar. 04 ] Available from: https://arxiv.org/pdf/1612.03672.pdf - 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
- 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
- The star formation rate in Milky Way: results from stars and planetary nebulae
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