Gravitational instability of filamentary molecular clouds, including ambipolar diffusion; Non-isothermal filament
Mohammad Hosseinirad, Shahram Abbassi, Mahmood Roshan, Kazem Naficy

TL;DR
This study investigates how non-isothermal equations of state, magnetic fields, and ambipolar diffusion influence the gravitational stability of filamentary molecular clouds, revealing that softer states and ambipolar diffusion tend to destabilize these structures.
Contribution
It compares the effects of logatropic and polytropic equations of state on filament stability, incorporating magnetic fields and ambipolar diffusion within a non-ideal MHD framework.
Findings
Softer equations of state increase instability in absence of magnetic fields.
Moderate magnetic fields enhance filament stability depending on the equation of state.
Ambipolar diffusion generally destabilizes filamentary structures.
Abstract
Recent observations of the filamentary molecular clouds show that their properties deviate from the isothermal equation of state. Theoretical investigations proposed that the logatropic and the polytropic equations of state with negative indexes can provide a better description for these filamentary structures. Here, we aim to compare the effects of these softer non-isothermal equation of states with their isothermal counterpart on the global gravitational instability of a filamentary molecular cloud. By incorporating the ambipolar diffusion, we use the non-ideal magnetohydrodynamics framework for a filament that is threaded by a uniform axial magnetic field. We perturb the fluid and obtain the dispersion relation both for the logatropic and polytropic equations of state by taking the effects of magnetic field and ambipolar diffusion into account. Our results suggest that, in absence of…
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