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December 8, 2025Monthly Notices of the Royal Astronomical SocietyOpen Access

OPTICAM Reveals Hints of Cyclotron Emission from the Intermediate Polar V709 Cas

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Authors

ZIZ A IrvingNSNoel Castro SeguraDAD. Altamirano

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Overview

Observational analysis reveals cyclotron radiation signatures in V709 Cas, highlighting its magnetic field characteristics.

Key Points

  • X-ray and near-infrared observations indicate cyclotron radiation from V709 Cas, suggesting it adds to known cyclotron-emitting IPs.
  • Periodogram analysis of light curves shows features at the spin, but not the spin-orbit beat, pinpointing sources of cyclotron emissions.
  • OPTICAM captured simultaneous photometry in multiple bands over late 2024, aligning with NICER observations.
  • Findings point to a magnetic field strength range of 10 MG to 40 MG, calling for further studies on magnetism in cataclysmic variables.

Cite This Study

Irving et al. (2025) studied this question.

synapsesocial.com/papers/694020e22d562116f28faa06https://doi.org/10.1093/mnras/staf2177
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