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20162024
most citedGravitational instability of filamentary molecular clouds, including ambipolar diffusion

19 citations · 41 across the 6 of their papers we have counts for

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Showing astro-ph.GAShow all

5 papers · 1 filter

astro-ph.GA2024★ 6 cited

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…

astro-ph.GA2023★ 3 cited

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…

astro-ph.GA2021

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…

astro-ph.GA2017★ 8 cited

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…

astro-ph.GA2016★ 19 cited

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…