A. Bertrand - Home pages of ESAT - KU Leuven
For high dust temperatures (Td>3500Co), thermal electron emission can dominate, resulting in a positive charging of the particle surface ( ...
The ALMA REBELS Survey: cosmic dust temperature evolution out ...(2)), the optical depth reaches unity at a wavelength of ?0 = c/?0 = 170 ± 23 µm with a dust temperature of Td = 52 ± 5 K, which is fully ... Constraints on the nature of dust particles by infrared observationsAbstract. We have computed the dust temperature distribution to be expected in a pre?protostellar core in the phase prior to the onset of gravitational ... Retrieval of microphysical properties of dust aerosols from extinction ...temperatures: ? 1 eV for SEE electrons and the dust surface temperature Td (? 10?2 ?. 10?1 eV) for THE electrons. Consequently, their gyroradii ?Lse are ...
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