New VLA observations catch about 90 percent circularly polarized, drifting radio bursts from DG CVn, suggesting electron cyclotron maser emission tied to the binary's fast rotation.
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Polarized, variable radio emission from the scallop-shell binary system DG CVn
New VLA observations catch about 90 percent circularly polarized, drifting radio bursts from DG CVn, suggesting electron cyclotron maser emission tied to the binary's fast rotation.