Coherent and Incoherent Emission from the Ordered Magnetospheres of Low-Mass Stars, UCDs, and Massive Stars
F. Cavallaro, P. Leto, Barnali Das, Corrado Trigilio et autres
Massive early-type (B/A) stars and ultracool dwarfs (UCDs) represent two distinct regimes in which ordered, large-scale magnetospheres are observed. In rapidly rotating massive stars, incoherent radio emission is explained by the centrifugal breakout (CBO) mechanism: plasma confined within the rigidly rotating magnetosphere …
it, in, au, nl, sk, us, cl (code pays fourni par la source)
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arXiv (Cornell University)