Simulation of the rotation-modulated and satellite-induced radio emissions from brown dwarfs

Details Simulation of the rotation-modulated and satellite-induced radio emissions from brown dwarfs Simulation of the rotation-modulated and satellite-induced radio emissions from brown dwarfs

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf...90k&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.90

Physics

Scientific paper

We simulate the dynamic spectra of the radio emission from a brown dwarf. The emission is produced due to the electron-cyclotron maser instability. Two source models are considered: the emission caused by interaction with a satellite and the emission from a sector of active longitudes. We have found that for the dwarf TVLM513 the model of an active sector (with a highly tilted magnetic dipole) fits the observations better.

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