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MHD numerical simulations of proto-stellar jets

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Abstract

We will summarize in this paper the effects that the presence of the magnetic field can cause to proto-stellar jet dynamics, structure and emission line properties, and the differences between two- and three-dimensional numerical simulations will be emphasized.

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Authors and Affiliations

  1. Departamento de Ciências Exatas e Tecnológicas, Rodovia Ilhéus-Itabuna, Universidade Estadual de Santa Cruz, km 16, Ilhéus, Bahia, Brazil, CEP 45650-000

    Adriano Hoth Cerqueira & Elisabete M. de Gouveia Dal Pino

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  1. Adriano Hoth Cerqueira
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  2. Elisabete M. de Gouveia Dal Pino
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Cerqueira, A.H., de Gouveia Dal Pino, E.M. MHD numerical simulations of proto-stellar jets. Space Science Reviews 107, 337–340 (2003). https://doi.org/10.1023/A:1025577218042

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