The star formation rate in Milky Way: results from stars and planetary nebulae (2011)
- Authors:
- USP affiliated authors: MACIEL, WALTER JUNQUEIRA - IAG ; COSTA, ROBERTO DELL' AGLIO DIAS DA - IAG
- Unidade: IAG
- Subjects: FORMAÇÃO DE ESTRELAS; GALÁXIA (VIA LÁCTEA)
- Language: Inglês
- Imprenta:
- Publisher: International Astronomical Union
- Publisher place: Paris
- Date published: 2011
- Source:
- Conference titles: IAU Symposium
-
ABNT
MACIEL, Walter Junqueira e ROCHA-PINTO, H. J. e COSTA, Roberto Dell'Aglio Dias da. The star formation rate in Milky Way: results from stars and planetary nebulae. 2011, Anais.. Paris: International Astronomical Union, 2011. . Acesso em: 23 jan. 2026. -
APA
Maciel, W. J., Rocha-Pinto, H. J., & Costa, R. D. 'A. D. da. (2011). The star formation rate in Milky Way: results from stars and planetary nebulae. In The spectral energy distribution of galaxies (SED 2011): Abstracts. Paris: International Astronomical Union. -
NLM
Maciel WJ, Rocha-Pinto HJ, Costa RD'AD da. The star formation rate in Milky Way: results from stars and planetary nebulae. The spectral energy distribution of galaxies (SED 2011): Abstracts. 2011 ;[citado 2026 jan. 23 ] -
Vancouver
Maciel WJ, Rocha-Pinto HJ, Costa RD'AD da. The star formation rate in Milky Way: results from stars and planetary nebulae. The spectral energy distribution of galaxies (SED 2011): Abstracts. 2011 ;[citado 2026 jan. 23 ] - 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
- 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
- A evolução química da Via Láctea com fluxos radiais de gás
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