V. Alexiades, G. Amiez, and P. A. Gremaud, Super-time-stepping acceleration of explicit schemes for parabolic problems, Communications in Numerical Methods in Engineering, vol.77, issue.1, p.31, 1996.
DOI : 10.1002/(SICI)1099-0887(199601)12:1<31::AID-CNM950>3.0.CO;2-5

C. Argiroffi, A. Maggio, G. Peres, C. Argiroffi, A. Maggio et al., X-ray emission from MP??Muscae: an old classical T Tauri star, Astronomy and Astrophysics, vol.465, issue.1, pp.5-939, 2007.
DOI : 10.1051/0004-6361:20067016

D. S. Balsara and D. S. Spicer, A Staggered Mesh Algorithm Using High Order Godunov Fluxes to Ensure Solenoidal Magnetic Fields in Magnetohydrodynamic Simulations, Journal of Computational Physics, vol.149, issue.2, p.270, 1999.
DOI : 10.1006/jcph.1998.6153

N. Calvet and E. Gullbring, The Structure and Emission of the Accretion Shock in T Tauri Stars, The Astrophysical Journal, vol.509, issue.2, p.802, 1998.
DOI : 10.1086/306527

R. L. Curran, C. Argiroffi, and G. G. Sacco, Multiwavelength diagnostics of accretion in an X-ray selected sample of CTTSs, Astronomy & Astrophysics, vol.526, p.104, 2011.
DOI : 10.1051/0004-6361/201015522

J. Donati, M. M. Jardine, and S. G. Gregory, Magnetospheric accretion on the T Tauri star BP Tauri, Monthly Notices of the Royal Astronomical Society, vol.386, issue.3, p.1234, 2008.
DOI : 10.1111/j.1365-2966.2008.13111.x
URL : https://hal.archives-ouvertes.fr/hal-00398497

J. Donati, M. B. Skelly, and J. Bouvier, Magnetospheric accretion and spin-down of the prototypical classical T Tauri star AA Tau, Monthly Notices of the Royal Astronomical Society, vol.409, issue.4, p.1347, 2010.
DOI : 10.1111/j.1365-2966.2010.17409.x
URL : https://hal.archives-ouvertes.fr/hal-00632018

J. J. Drake, B. Ercolano, E. Flaccomio, G. Micela, A. K. Dupree et al., X-RAY PHOTOEVAPORATION-STARVED T TAURI ACCRETION, The Astrophysical Journal, vol.699, issue.1, pp.35-73, 2009.
DOI : 10.1088/0004-637X/699/1/L35
URL : http://arxiv.org/abs/0905.1690

E. Flaccomio, F. Damiani, and G. Micela, X???Ray Observation of the Orion Nebula Cluster. II. Relationship between X???Ray Activity Indicators and Stellar Parameters, The Astrophysical Journal, vol.582, issue.1, p.398, 2003.
DOI : 10.1086/344536

S. G. Gregory, K. Wood, M. Jardine, H. M. Günther, J. H. Schmitt et al., Why are accreting T Tauri stars observed to be less luminous in X-rays than non-accretors?, Monthly Notices of the Royal Astronomical Society: Letters, vol.379, issue.1, pp.35-1111, 2007.
DOI : 10.1111/j.1745-3933.2007.00328.x

C. M. Johns-krull, The Magnetic Fields of Classical T Tauri Stars, The Astrophysical Journal, vol.664, issue.2, p.975, 2007.
DOI : 10.1086/519017

T. Matsakos, J. Chièze, and C. Stehlé, YSO accretion shocks: magnetic, chromospheric or stochastic flow effects can suppress fluctuations of X-ray emission, Astronomy & Astrophysics, vol.557, issue.170, pp.69-228, 2007.
DOI : 10.1051/0004-6361/201321820
URL : https://hal.archives-ouvertes.fr/cea-01135429

T. Miyoshi and K. Kusano, A multi-state HLL approximate Riemann solver for ideal magnetohydrodynamics, Journal of Computational Physics, vol.208, issue.1, p.315, 2005.
DOI : 10.1016/j.jcp.2005.02.017

S. Orlando, Y. Lou, R. Rosner, and G. Peres, Propagation of three-dimensional Alfv??n waves in a stratified, thermally conducting solar wind, Journal of Geophysical Research: Space Physics, vol.325, issue.23, p.24443, 1996.
DOI : 10.1029/96JA02304

S. Orlando, F. Bocchino, F. Reale, G. Peres, and P. Pagano, The Importance of Magnetic???Field???Oriented Thermal Conduction in the Interaction of SNR Shocks with Interstellar Clouds, The Astrophysical Journal, vol.678, issue.1, p.274, 2008.
DOI : 10.1086/529420

T. Preibisch, Y. Kim, and F. Favata, Orion Ultradeep Project, The Astrophysical Journal Supplement Series, vol.160, issue.2, p.401, 2005.
DOI : 10.1086/432891
URL : https://hal.archives-ouvertes.fr/hal-00398188

F. Reale, S. Orlando, and P. Testa, Bright Hot Impacts by Erupted Fragments Falling Back on the Sun: A Template for Stellar Accretion, Science, vol.341, issue.6143, p.251, 2013.
DOI : 10.1126/science.1235692

G. G. Sacco, C. Argiroffi, and S. Orlando, X-ray emission from dense plasma in classical T Tauri stars: hydrodynamic modeling of the accretion shock, Astronomy and Astrophysics, vol.491, issue.2, pp.17-91, 2001.
DOI : 10.1051/0004-6361:200810753

L. Spitzer, Physics of Fully Ionized Gases, American Journal of Physics, vol.31, issue.11, 1962.
DOI : 10.1119/1.1969155

K. G. Stassun, D. R. Ardila, M. Barsony, G. Basri, and R. D. Mathieu, X-Ray Properties of Pre-Main-Sequence Stars in the Orion Nebula Cluster with Known Rotation Periods, The Astronomical Journal, vol.127, issue.6, p.3537, 2004.
DOI : 10.1086/420989

A. Telleschi, M. Güdel, K. R. Briggs, M. Audard, and L. Scelsi, High-resolution X-ray spectroscopy of T??Tauri stars in the??Taurus-Auriga complex, Astronomy and Astrophysics, vol.468, issue.2, p.443, 2007.
DOI : 10.1051/0004-6361:20066193