Source: Monthly Notices of the Royal Astronomical Society. Unidades: IAG, EACH
Subjects: ESTRELAS, ESTRELAS BINÁRIAS, VENTO
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FALCETA-GONÇALVES, D e ABRAHAM, Zulema. MHD numerical simulations of colliding winds in massive binary systems: I. Thermal versus non-thermal radio emission. Monthly Notices of the Royal Astronomical Society, v. 423, p. 1562-1570, 2012Tradução . . Disponível em: https://doi.org/10.1111/j.1365-2966.2012.20978.x. Acesso em: 30 jul. 2024.APA
Falceta-Gonçalves, D., & Abraham, Z. (2012). MHD numerical simulations of colliding winds in massive binary systems: I. Thermal versus non-thermal radio emission. Monthly Notices of the Royal Astronomical Society, 423, 1562-1570. doi:10.1111/j.1365-2966.2012.20978.xNLM
Falceta-Gonçalves D, Abraham Z. MHD numerical simulations of colliding winds in massive binary systems: I. Thermal versus non-thermal radio emission [Internet]. Monthly Notices of the Royal Astronomical Society. 2012 ; 423 1562-1570.[citado 2024 jul. 30 ] Available from: https://doi.org/10.1111/j.1365-2966.2012.20978.xVancouver
Falceta-Gonçalves D, Abraham Z. MHD numerical simulations of colliding winds in massive binary systems: I. Thermal versus non-thermal radio emission [Internet]. Monthly Notices of the Royal Astronomical Society. 2012 ; 423 1562-1570.[citado 2024 jul. 30 ] Available from: https://doi.org/10.1111/j.1365-2966.2012.20978.x
