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A schematic sketch of the evolution in star-disk interaction.
Magnetospheric Accretion and Ejection of Matter in Resistive Magnetohydrodynamic Simulations
In numerical simulations of the star-disk system, after the relaxation, the disk is truncated at the truncation radius R_t. Position of the R_t is close to the line of balance of the disk ram pressure and the magnetic pressure, which is located between a central object and the disk inner radius.
Magnetospheric Accretion and Ejection of Matter in Resistive MHD Simulations
Cemeljic, Miljenko
Visiting Assistant Research Fellow
photo of Cemeljic, Miljenko
Office: ASMAB 1218
TEL: +886-2-2366-5406
FAX: +886-2-2367-7849

Education and Positions

  • ASIAA/TIARA, Hsinchu, Taiwan (2007 ~ 2008)
  • Marie Curie research Fellow, JETSET collaboration, University of Athens, Greece (2005 ~ 2007)
  • Astrophysikalisches Institut Potsdam, Germany (1999 ~ 2003)
  • Nicolaus Copernicus Astronomical Center, Warsaw, Poland (1997 ~ 1999)
  • University of Potsdam, Germany, PhD (2000 ~ 2005)
  • University of Zagreb, Croatia, MS (1988 ~ 1996)

Research Interests

MHD Simulations

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