Explaining the features of the bipolar nebula Eta Carinae gas dynamical simulations (2005)
Source: Proceedings. Conference titles: Conference on the Fate of the Most Massive Stars. Unidade: IAG
Subjects: NEBULOSAS, ESTRELAS, COSMOLOGIA
ABNT
DAL PINO, Elisabete Maria de Gouveia et al. Explaining the features of the bipolar nebula Eta Carinae gas dynamical simulations. 2005, Anais.. San Francisco: Astronomical Society of the Pacific, 2005. . Acesso em: 15 nov. 2024.APA
Dal Pino, E. M. de G., González, R. F., Raga, A. C., & Velezquez, P. F. (2005). Explaining the features of the bipolar nebula Eta Carinae gas dynamical simulations. In Proceedings. San Francisco: Astronomical Society of the Pacific.NLM
Dal Pino EM de G, González RF, Raga AC, Velezquez PF. Explaining the features of the bipolar nebula Eta Carinae gas dynamical simulations. Proceedings. 2005 ;[citado 2024 nov. 15 ]Vancouver
Dal Pino EM de G, González RF, Raga AC, Velezquez PF. Explaining the features of the bipolar nebula Eta Carinae gas dynamical simulations. Proceedings. 2005 ;[citado 2024 nov. 15 ]