Result Number | Material Type | Add to My Shelf Action | Record Details and Options |
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1 |
Material Type: Artigo
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3D MHD modeling of the expanding remnant of SN 1987A: Role of magnetic field and non-thermal radio emissionOrlando, S. ; Miceli, M. ; Petruk, O. ; Ono, M. ; Nagataki, S. ; Aloy, M. A. ; Mimica, P. ; Lee, S.-H. ; Bocchino, F. ; Peres, G. ; Guarrasi, M.Astronomy and astrophysics (Berlin), 2019-02, Vol.622, p.A73 [Periódico revisado por pares]Texto completo disponível |
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2 |
Material Type: Artigo
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3D MHD modeling of the expanding remnant of SN 1987AOrlando, S. ; Miceli, M. ; Petruk, O. ; Ono, M. ; Nagataki, S. ; Aloy, M. A. ; Mimica, P. ; Lee, S.-H. ; Bocchino, F. ; Peres, G. ; Guarrasi, M.Astronomy and astrophysics (Berlin), 2019-02, Vol.622 [Periódico revisado por pares]Heidelberg: EDP SciencesTexto completo disponível |
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3 |
Material Type: Artigo
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YSO accretion shocks: magnetic, chromospheric or stochastic flow effects can suppress fluctuations of X-ray emissionMatsakos, T. ; Chièze, J.-P. ; Stehlé, C. ; González, M. ; Ibgui, L. ; de Sá, L. ; Lanz, T. ; Orlando, S. ; Bonito, R. ; Argiroffi, C. ; Reale, F. ; Peres, G.Astronomy and astrophysics (Berlin), 2013-09, Vol.557, p.np-np [Periódico revisado por pares]EDP SciencesTexto completo disponível |
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4 |
Material Type: Artigo
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Three-dimensional modeling from the onset of the SN to the full-fledged SNR: Role of an initial ejecta anisotropy on matter mixingTutone, A. ; Orlando, S. ; Miceli, M. ; Ustamujic, S. ; Ono, M. ; Nagataki, S. ; Ferrand, G. ; Greco, E. ; Peres, G. ; Warren, D. C. ; Bocchino, F.Astronomy and astrophysics (Berlin), 2020-10, Vol.642, p.A67 [Periódico revisado por pares]Texto completo disponível |
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5 |
Material Type: Artigo
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Radiative accretion shocks along nonuniform stellar magnetic fields in classical T Tauri starsOrlando, S. ; Bonito, R. ; Argiroffi, C. ; Reale, F. ; Peres, G. ; Miceli, M. ; Matsakos, T. ; Stehlé, C. ; Ibgui, L. ; de Sa, L. ; Chièze, J. P. ; Lanz, T.Astronomy and astrophysics (Berlin), 2013-11, Vol.559, p.np-np [Periódico revisado por pares]EDP SciencesTexto completo disponível |