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Home Seminarios SEMINARIO DFI: The radio continuum emission mechanisms from interstellar molecular clouds
SEMINARIO DFI: The radio continuum emission mechanisms from interstellar molecular clouds Imprimir
Expositor: Simón Casassus
Departamento de Astronomía---FCFM

Viernes 4 de Noviembre, 16:00 h
Sala F12

Abstract: An `anomalous' radio continuum was found 10 years ago in the direction
of molecular clouds. This emission is consistent with electric dipole
radiation from polarized very small grains spinning at GHz frequencies,
or `spinning dust'. I will summarise recent observations of this
phenomenon, and investigate the nature of the grain spin-up
mechanism. The data so far are consistent with spin-up from the recoil
of H2 formation on grain surfaces, and are not consistent with radiative
torques or collisions.

 

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