UR #26: Measuring the Radio Corona of Young M Dwarf Stars
Today’s undergraduate research post features a student who used radio images of red dwarf stars to tease out clues about the particle acceleration in their coronae.
Today’s undergraduate research post features a student who used radio images of red dwarf stars to tease out clues about the particle acceleration in their coronae.
Forbich, Berger, and Reid attempt to use a large radio array to detect stellar wobbles induced by orbiting planets at larger separations than are usually probed