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- W2063849628 abstract "Abstract The condensation mode of thermal instability is studied as a possible mechanism of interstellar cloud formation. It is shown that perturbations with characteristic dynamical time smaller than the cooling time evolve to develop hydrodynamical motions corresponding in general to the acoustic mode which prevents perturbations to condense quietly into clouds. The condensation mode is shown to be driven by thermal instability for a special choice of initial conditions for hydrodynamic variables. Perturbations of sufficiently large wavelength are shown to evolve to a dynamical state similar to the condensation mode independently of the form of the initial perturbations. Possible applications to the interstellar gas and the gas of cooling flows are indicated." @default.
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- W2063849628 date "1996-11-01" @default.
- W2063849628 modified "2023-09-26" @default.
- W2063849628 title "On interstellar cloud formation due to thermal instability" @default.
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- W2063849628 doi "https://doi.org/10.1080/10556799608205473" @default.
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