Leto P.; Trigilio C.; Buemi C.S.; Leone F.; Pillitteri I.; Fossati L.; Cavallaro F.; Oskinova L.M.; Ignace R.; Krtička J.; Umana G.; Catanzaro G.; Ingallinera A.; Bufano F.; Riggi S.; Cerrigone L.; Loru S.; Schilliró F.; Agliozzo C.; Phillips N.M.; Giarrusso M.; Robrade J.
(2020)
© 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. The non-thermal radio emission of main-sequence early-type stars is a signature of stellar magnetism. We present ...