The evolution of the radial gradient of oxygen abundance in spiral galaxies (2017)
- Authors:
- USP affiliated authors: MACIEL, WALTER JUNQUEIRA - IAG ; COSTA, ROBERTO DELL'AGLIO DIAS DA - IAG
- Unidade: IAG
- Assunto: GALÁXIAS ESPIRAIS
- 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
MOLLÁ, M. et al. The evolution of the radial gradient of oxygen abundance in spiral galaxies. 2017, Anais.. Ithaca, N.Y.: Cornell University, 2017. Disponível em: https://arxiv.org/pdf/1612.03348.pdf. Acesso em: 23 jan. 2026. -
APA
Mollá, M., Díaz, A. I., Ascasibar, Y., Gibson, B. K., Cavichia, O., Costa, R. D. 'A. D. da, & Maciel, W. J. (2017). The evolution of the radial gradient of oxygen abundance in spiral galaxies. In ARXIV. Ithaca, N.Y.: Cornell University. Recuperado de https://arxiv.org/pdf/1612.03348.pdf -
NLM
Mollá M, Díaz AI, Ascasibar Y, Gibson BK, Cavichia O, Costa RD'AD da, Maciel WJ. The evolution of the radial gradient of oxygen abundance in spiral galaxies [Internet]. ARXIV. 2017 ;[citado 2026 jan. 23 ] Available from: https://arxiv.org/pdf/1612.03348.pdf -
Vancouver
Mollá M, Díaz AI, Ascasibar Y, Gibson BK, Cavichia O, Costa RD'AD da, Maciel WJ. The evolution of the radial gradient of oxygen abundance in spiral galaxies [Internet]. ARXIV. 2017 ;[citado 2026 jan. 23 ] Available from: https://arxiv.org/pdf/1612.03348.pdf - 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
- Mass loss rates of Li-rich AGB/RGB stars
- The population of planetary nebulae near the Galactic Centre: chemical abundances
- Chemical evolution of the Galactic bulge: single and double infall models
- Nucleosynthesis of intermediate mass stars: inferences from the observed abundances in photoionized nebulae of the Local Group
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