Orlando, S. Bonito, R. Argiroffi, C. Reale, F. Peres, G. Miceli, M. Matsakos, T. Stehlé, C. Ibgui, L. de Sa, L.
...

Context. According to the magnetospheric accretion model, hot spots form on the surface of classical T Tauri stars (CTTSs) in regions where accreting disk material impacts the stellar surface at supersonic velocity, generating a shock.Aims. We investigate the dynamics and stability of postshock plasma that streams along nonuniform stellar magnetic ...

Orlando, S. Bonito, R. Argiroffi, C. Reale, F. Peres, G. Miceli, M. Matsakos, T. Stehlé, C. Ibgui, L. de Sa, L.
...

Context. According to the magnetospheric accretion model, hot spots form on the surface of classical T Tauri stars (CTTSs) in regions where accreting disk material impacts the stellar surface at supersonic velocity, generating a shock.Aims. We investigate the dynamics and stability of postshock plasma that streams along nonuniform stellar magnetic ...

Orlando, S. Bonito, R. Argiroffi, C. Reale, F. Peres, G. Miceli, M. Matsakos, T. Stehlé, C. Ibgui, L. de Sa, L.
...

Context. According to the magnetospheric accretion model, hot spots form on the surface of classical T Tauri stars (CTTSs) in regions where accreting disk material impacts the stellar surface at supersonic velocity, generating a shock.Aims. We investigate the dynamics and stability of postshock plasma that streams along nonuniform stellar magnetic ...

Orlando, S. Bonito, R. Argiroffi, C. Reale, F. Peres, G. Miceli, M. Matsakos, T. Stehlé, C. Ibgui, L. de Sa, L.
...

Context. According to the magnetospheric accretion model, hot spots form on the surface of classical T Tauri stars (CTTSs) in regions where accreting disk material impacts the stellar surface at supersonic velocity, generating a shock.Aims. We investigate the dynamics and stability of postshock plasma that streams along nonuniform stellar magnetic ...

Orlando, S. Bonito, R. Argiroffi, C. Reale, F. Peres, G. Miceli, M. Matsakos, T. Stehlé, C. Ibgui, L. de Sa, L.
...

Context. According to the magnetospheric accretion model, hot spots form on the surface of classical T Tauri stars (CTTSs) in regions where accreting disk material impacts the stellar surface at supersonic velocity, generating a shock.Aims. We investigate the dynamics and stability of postshock plasma that streams along nonuniform stellar magnetic ...

Orlando, S. Bonito, R. Argiroffi, C. Reale, F. Peres, G. Miceli, M. Matsakos, T. Stehlé, C. Ibgui, L. de Sa, L.
...

Context. According to the magnetospheric accretion model, hot spots form on the surface of classical T Tauri stars (CTTSs) in regions where accreting disk material impacts the stellar surface at supersonic velocity, generating a shock.Aims. We investigate the dynamics and stability of postshock plasma that streams along nonuniform stellar magnetic ...

Orlando, S. Bonito, R. Argiroffi, C. Reale, F. Peres, G. Miceli, M. Matsakos, T. Stehlé, C. Ibgui, L. de Sa, L.
...

Context. According to the magnetospheric accretion model, hot spots form on the surface of classical T Tauri stars (CTTSs) in regions where accreting disk material impacts the stellar surface at supersonic velocity, generating a shock.Aims. We investigate the dynamics and stability of postshock plasma that streams along nonuniform stellar magnetic ...

Orlando, S. Bonito, R. Argiroffi, C. Reale, F. Peres, G. Miceli, M. Matsakos, T. Stehlé, C. Ibgui, L. de Sa, L.
...

Context. According to the magnetospheric accretion model, hot spots form on the surface of classical T Tauri stars (CTTSs) in regions where accreting disk material impacts the stellar surface at supersonic velocity, generating a shock.Aims. We investigate the dynamics and stability of postshock plasma that streams along nonuniform stellar magnetic ...

Orlando, S. Bonito, R. Argiroffi, C. Reale, F. Peres, G. Miceli, M. Matsakos, T. Stehlé, C. Ibgui, L. de Sa, L.
...

Context. According to the magnetospheric accretion model, hot spots form on the surface of classical T Tauri stars (CTTSs) in regions where accreting disk material impacts the stellar surface at supersonic velocity, generating a shock.Aims. We investigate the dynamics and stability of postshock plasma that streams along nonuniform stellar magnetic ...

Orlando, S. Bonito, R. Argiroffi, C. Reale, F. Peres, G. Miceli, M. Matsakos, T. Stehlé, C. Ibgui, L. de Sa, L.
...

Context. According to the magnetospheric accretion model, hot spots form on the surface of classical T Tauri stars (CTTSs) in regions where accreting disk material impacts the stellar surface at supersonic velocity, generating a shock.Aims. We investigate the dynamics and stability of postshock plasma that streams along nonuniform stellar magnetic ...