Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21722303h&link_type=abstract
American Astronomical Society, AAS Meeting #217, #223.03; Bulletin of the American Astronomical Society, Vol. 43, 2011
Astronomy and Astrophysics
Astronomy
Scientific paper
One of the most significant discoveries in stellar radio astronomy was the confirmation that cool dwarf flare stars can be persistent sources of non-thermal radio emission. With the commissioning of the EVLA, the potential exists to finally fully understand the means by which such non-thermal coronae are generated and sustained. Along with the expected increase in the sample of known objects, the capability to achieve continuous spectra covering 1-50 GHz, enables a robust assessment of the emission processes involved in the associated radio emissions. These observations can be coupled with recently developed spectropolarimetric techniques to simultaneous assess the strength and configuration of the magnetic fields. I will discuss plans to commence such observations as well as studies of radio emissions from brown dwarfs and exoplanets achievable with EVLA and LOFAR respectively.
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