MHD numerical simulations of Perseus A: formation of filaments and magnetic loops (2009)
Source: Cosmic magnetic fields: from planets, to stars and galaxies. Conference titles: IAU Symposium. Unidade: IAG
Subjects: GALÁXIAS, AGLOMERADOS DE GALÁXIAS, MÉTODOS NUMÉRICOS
ABNT
GONÇALVES, Diego Falceta e DAL PINO, Elisabete Maria de Gouveia e GALLAGHER III, J. MHD numerical simulations of Perseus A: formation of filaments and magnetic loops. 2009, Anais.. Paris: IAU, 2009. . Acesso em: 15 out. 2024.APA
Gonçalves, D. F., Dal Pino, E. M. de G., & Gallagher III, J. (2009). MHD numerical simulations of Perseus A: formation of filaments and magnetic loops. In Cosmic magnetic fields: from planets, to stars and galaxies. Paris: IAU.NLM
Gonçalves DF, Dal Pino EM de G, Gallagher III J. MHD numerical simulations of Perseus A: formation of filaments and magnetic loops. Cosmic magnetic fields: from planets, to stars and galaxies. 2009 ;[citado 2024 out. 15 ]Vancouver
Gonçalves DF, Dal Pino EM de G, Gallagher III J. MHD numerical simulations of Perseus A: formation of filaments and magnetic loops. Cosmic magnetic fields: from planets, to stars and galaxies. 2009 ;[citado 2024 out. 15 ]