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- W2080924738 abstract "Exact analytic solutions are presented for equilibrium states of a self-gravitating one-dimensional cloud of gas, embedded in an external gravitational field due to a plane of 'stars' being heated at a rate proportional to the local gas density, and cooling by thermal conduction. It is found that the general topology of the solutions is such that the gas density has a minimum on the plane of 'stars', rising to an infinite but integrable peak away from the plane so that the total mass of gas in the cloud is finite. The results may be of interest in investigations of interstellar molecular clouds and of filamentary structures in supernova remnants as well as in the modeling of gas distributions around 'cocoon' protostars." @default.
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- W2080924738 date "1980-12-01" @default.
- W2080924738 modified "2023-09-27" @default.
- W2080924738 title "On equilibrium states of heated self-gravitating gas clouds cooling by conduction in an external gravitational field" @default.
- W2080924738 doi "https://doi.org/10.1086/158547" @default.
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