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- W2101137313 abstract "Abstract In molecular clouds the dust charge can be determined by non-thermal electrons from cosmic-ray ionization. If the energy of the non-thermal electrons is E≥2 keV and their fraction is only 10−3–10−4 of the thermal electrons in a molecular gas, the grain charge can be as high as | z | ≈ 10 in the range of gas densities n≈ 105–106 cm−3. In the high-density range n>106 cm−3, the grain charge approaches the thermal limit | z | ≈ 0.3." @default.
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- W2101137313 date "2007-10-01" @default.
- W2101137313 modified "2023-10-18" @default.
- W2101137313 title "Charging of dust particles in molecular clouds" @default.
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- W2101137313 doi "https://doi.org/10.1080/10556790601156667" @default.
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