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- W1966791356 abstract "We investigate the equilibrium properties of self-gravitating magnetized clouds with polytropic equations of state with negative index n. In particular, we consider scale-free isopedic configurations that have constant dimensionless spherical mass-to-flux ratio λr and that may constitute pivotal states for subsequent dynamical collapse to form groups or clusters of stars. For given Γ = 1 + 1/n, equilibria with smaller values of λr are more flattened, ranging from spherical configurations with λr = ∞ to completely flattened states for λr = 1. For a given amount of support provided by the magnetic field as measured by the dimensionless parameter H0, equilibria with smaller values of Γ are more flattened. However, logatropic (defined by Γ = 0) disks do not exist. The only possible scale-free isopedic equilibria with logatropic equation of state are spherical uniformly magnetized clouds." @default.
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- W1966791356 date "1999-08-20" @default.
- W1966791356 modified "2023-09-26" @default.
- W1966791356 title "Scale‐free Equilibria of Isopedic Polytropic Clouds" @default.
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- W1966791356 doi "https://doi.org/10.1086/307579" @default.
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