2 papers
astro-ph.SR2024
Radio emission from the magnetically active M dwarf UV Ceti from 1 GHz to 105 GHz
Kathryn Plant, Gregg Hallinan, Tim Bastian
BL and UV Ceti are a nearby (2.7 pc) binary system with similar masses, spectral types, and rapid rotation rates, but very different magnetic activity. UV Ceti's much stronger larg…
astro-ph.SR2022
Radio Emission from UV Cet: Auroral Emission from a Stellar Magnetosphere
Timothy Bastian, Bill Cotton, Gregg Hallinan
The archetypical flare star UV Cet was observed by MeerKAT on 5-6 October 2021. A large radio outburst with a duration of hr was observed between 886-1682 MHz with a time…