astro-ph 9401010 RADIO EMITTING DUST IN THE FREE ELECTRON LAYER OF SPIRAL GALAXIES: TESTING THE DISK/HALO INTERFACE

We present a study of the radio emission from rotating, charged dust grains immersed in the ionized gas constituting the thick, H -emitting disk of many spiral galaxies. Using upto-date optical constants, the charge on the grains exposed to the di use galactic UV ux has been calculated. An analytical approximation for the grain charge has been derived, which is then used to obtain the grain rotation frequency. Grains are found to have substantial radio emission peaked at a cuto frequency in the range 10-100 GHz, depending on the grain size distribution and on the e ciency of the radiative damping of the grain rotation. The dust radio emission is compared to the free-free emission from the ionized gas component; some constraints on the magnetic eld strength in the observed dusty laments are also discussed. The model can be used to test the disk-halo interface environment in spiral galaxies, to determine the amount and size distribution of dust in their ionized component, and to investigate the rotation mechanisms for the dust. Numerical estimates are given for experimental purposes.