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- W2110740566 abstract "The efficiency of the transfer of energy from supernovae into interstellar cloud motions is investigated. A lower limit of about 0·002 is obtained, but values near 0·01 are more likely. Taking all uncertainties in the theory and observations into account, the energy per supernova, in the form of relativistic particles or high-velocity matter, needed to maintain the random motions in the interstellar gas is estimated as 10 51·4±1 ergs." @default.
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- W2110740566 date "1967-01-01" @default.
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- W2110740566 title "Supernovae and interstellar gas dynamics" @default.
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- W2110740566 doi "https://doi.org/10.1017/s0074180900100774" @default.
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