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- W1991488908 abstract "Stellar winds from O and WR stars transfer large amounts of mechanical energy and momentum into the interstellar medium. They sweep up and compress the interstellar material, creating interstellar bubbles. These structures are detected as optical ring nebulae, as thermal radio continuum sources, as infrared shells, as neutral gas voids and expanding shells in the H I line emission distribution, and as molecular shells." @default.
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- W1991488908 date "2006-08-01" @default.
- W1991488908 modified "2023-10-18" @default.
- W1991488908 title "Stellar formation in HI interstellar bubbles around massive stars" @default.
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- W1991488908 doi "https://doi.org/10.1017/s1743921307002323" @default.
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