117 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Ferdowsi University of MashhadIR10 papers
- Research Institute for Astronomy and Astrophysics of MaraghIR7 papers
- Institute for Research in Fundamental SciencesIR6 papers
- Damghan UniversityIR5 papers
- Golestan University of Medical SciencesIR2 papers
- Jahrom University of Medical SciencesIR2 papers
- Kashan University of Medical SciencesIR2 papers
- Mashhad University of Medical SciencesIR2 papers
- Max Planck Institute for AstronomyDE2 papers
- Payame Noor UniversityIR2 papers
- Russian Academy of SciencesRU2 papers
- Schmidt Institute of Physics of the EarthRU2 papers
5 papers · 2 filters
Properties of an accretion disc with a power-law stress-pressure relationship
Mohsen Shadmehri, Fazeleh Khajenabi, Sami Dib +1
Recent numerical simulations of magnetized accretion discs show that the radial-azimuthal component of the stress tensor due to the magnetorotational instability (MRI) is well repr…
Evolution of circumbinary protoplanetary disks with photoevaporative winds driven by External Far Ultraviolet Radiation
Mohsen Shadmehri, S. M. Ghoreyshi, N. Alipour
Lifetimes of protoplanetary disks (PPDs) are believed to be severely constrained by material depleting mechanisms, including photoevaporative winds due to the host star radiation o…
Magnetic Rayleigh-Taylor Instability in Radiative Flows
Asiyeh Yaghoobi, Mohsen Shadmehri
We present a linear analysis of the radiative Rayleigh-Taylor (RT) instability in the presence of magnetic field for both optically thin and thick regimes. When the flow is optical…
The local stability of the magnetized advection-dominated discs with the radial viscous force
S. M. Ghoreyshi, Mohsen Shadmehri
We study local stability of the advection-dominated optically thick (slim) and optically thin discs with purely toroidal magnetic field and the radial viscous force using a linear…
Structure of Protoplanetary Discs with Magnetically-driven Winds
Fazeleh Khajenabi, Mohsen Shadmehri, Martin E. Pessah +1
We present a new set of analytical solutions to model the steady state structure of a protoplanetary disc with a magnetically-driven wind. Our model implements a parametrization of…