19 citations · 41 across the 6 of their papers we have counts for
6 papers
The redshift evolution of galactic bar pattern speed in TNG50
Asiyeh Habibi, Mahmood Roshan, Mohammad Hosseinirad +4
In this paper, the redshift evolution of the galactic bar properties, like the bar length, pattern speed, and bar fraction, has been investigated for simulated galaxies at stellar…
Reconciling the magnetic field in central disc galaxies with the dynamical mass using the cosmological simulations
Mohammad Hosseinirad, Fatemeh Tabatabaei, Mojtaba Raouf +1
The Universe is pervaded by magnetic fields in different scales, although for simplicity, they are ignored in most cosmological simulations. In this paper, we use the TNG50, which…
Gravitational instability of non-isothermal filamentary molecular clouds, in presence of external pressure
Mohammad Mahdi Motiei, Mohammad Hosseinirad, Shahram Abbassi
Filamentary molecular clouds are omnipresent in the cold interstellar medium. Observational evidences show that the non-isothermal equations of state describe the filaments propert…
Capture rate of weakly interacting massive particles (WIMPs) in binary star systems
Ebrahim Hassani, Hossein Ebadi, Reza Pazhouhesh +1
The distribution of dark matter (DM) inside galaxies is not uniform. Near the central regions, its density is the highest. Then, it is logical to suppose that, inside galaxies, DM…
Gravitational instability of filamentary molecular clouds, including ambipolar diffusion; Non-isothermal filament
Mohammad Hosseinirad, Shahram Abbassi, Mahmood Roshan +1
Recent observations of the filamentary molecular clouds show that their properties deviate from the isothermal equation of state. Theoretical investigations proposed that the logat…
Gravitational instability of filamentary molecular clouds, including ambipolar diffusion
Mohammad Hosseinirad, Kazem Naficy, Shahram Abbassi +1
The gravitational instability of a filamentary molecular cloud in non-ideal magnetohydrodynamics is investigated. The filament is assumed to be in hydrostatic equilibrium. We add t…