RMxAA

Revista Mexicana de Astronomía y Astrofísica

ISSN: 3061-8649
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Keywords

ISM: clouds
ISM: kinematics and dynamics
stars: formation

How to Cite

The Properties and Stability of Self-Gravitating, Polytropic Spheres with γ = 1 to 1.4 Specific Heat Ratios. (2020). Revista Mexicana De Astronomía Y Astrofísica, 56(1), 55-62. https://doi.org/10.22201/ia.01851101p.2020.56.01.07

Abstract

We study self-gravitating, hydrostatic spheres with a polytropic equation of state P ∝ ργ (where γ is the specific heat ratio of the gas), considering structures with γ ≈ 1 as a model for molecular cloud cores with small departures from isothermality. We derive the properties (i.e., mass, radius and center to edge density ratio) as a function of γ for the maximal stable sphere through an application of "Bonnor's stability criterion". We find that in the γ = 1 → 4/3 range the mass of the maximal sphere (for a given central temperature) is almost constant, and that its radius and center to edge density ratio are growing functions of γ. We therefore have maximal stable, self-gravitating spheres with similar masses, but with increasing center to edge density contrasts for increasing departures from isothermality.
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