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- W42367837 abstract "Flow initiated in clumpy media can be radically different from those in smooth media. A particular class of flows relevant to such disparate objects as planetary nebulae and straburst galaxies arise when the clumps are concentrated around the flow initiation focus. We descride general features of such flows and comment on various astrophysical areas where they are of importance" @default.
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- W42367837 date "1992-01-01" @default.
- W42367837 modified "2023-10-16" @default.
- W42367837 title "Astronomical Bubbles with Clumpy Cores and Accelerating Haloes" @default.
- W42367837 hasPublicationYear "1992" @default.
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