Chemical evolution of the Magellanic Clouds based on planetary nebulae (2008)
Source: The Magellanic System : stars, gas, and galaxies : proceedings. Conference titles: IAU Symposium. Unidade: IAG
Subjects: NUVENS DE MAGALHÃES, ABUNDÂNCIAS (ASTRONOMIA), FORMAÇÃO E EVOLUÇÃO DA GALÁXIA, GALÁXIA (VIA LÁCTEA)
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: 29 set. 2024.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 2024 set. 29 ]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 2024 set. 29 ]