Electron cyclotron maser emission from ejected stellar prominences on V374 Peg
Abstract
ABSTRACT We investigate a possible origin for bursty radio emission observed on the active M dwarf V374 Peg, combining data-driven magnetic field modelling with archival radio light curves. We examine whether stellar prominence ejection can plausibly account for the observed radio bursts that have been attributed to electron cyclotron maser (ECM) emission. Our analysis shows that ejected prominences can produce the required energy range to drive the emission, and that modelled ECM visibility exhibits a rotational phase dependence consistent with the limited observational data (four observed bursts). The results support prominence ejection as a viable mechanism for ECM generation on V374 Peg and motivate further observational campaigns to constrain this process.
Fields of Study & Subjects
Pulsars and Gravitational Waves Research
Gamma-ray bursts and supernovae
Astrophysical Phenomena and Observations
Publication details
- Journal / source
- Monthly Notices of the Royal Astronomical Society
- Publisher
- Oxford University Press (OUP)
- Volume
- 546
- Issue
- 3
- Publication date
- 8 January 2026
- Language
- EN