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Understanding the Radio Emission from the β Cep Star V2187 Cyg

Authors: Luis F. Rodríguez,Susana Lizano,Jorge Cantó,Ricardo F. González,Mauricio Tapia
Publisher: American Astronomical Society
Publish date: 2025-1-3
ISSN: 0004-637X,1538-4357 DOI: 10.3847/1538-4357/ad9a69
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The authors convincingly propose a magnetic origin for the radio emission, but the reliance on indirect methods leaves room for ambiguity. Could you elaborate on why direct magnetic field measurements were not attempted, given their potential to confirm the gyrosynchrotron hypothesis?

The study assumes uniformity in wind dynamics and magnetic field structure. How might spatial variations in these parameters influence the interpretation of the radio pulse and spectral characteristics?

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