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- W2030007283 abstract "Grains ejected from stars at velocities of ∼ 107cm s−1 and/or grains accelerated by the pressure of starlight in the intercloud medium to velocities in the range 2 × 106 –107 cm s−1 are slowed to velocities of about 2 × 105 cm s−1 in a typical interstellar cloud. The interaction of fast grains with gas atoms as they are slowed in clouds could provide (a) the dominant heat source for interstellar clouds; (b) sites for molecule formation; and (c) a mechanism of providing a pressure balance between clouds and the intercloud medium.KeywordsStar FormationInterstellar MediumPressure BalanceMonthly NoticeInterstellar CloudThese keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves." @default.
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- W2030007283 date "1976-01-01" @default.
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- W2030007283 title "Effects of Suprathermal Grains" @default.
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- W2030007283 doi "https://doi.org/10.1007/978-94-010-1884-5_26" @default.
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