OPTICAM reveals hints of cyclotron emission from the intermediate polar V709 Cas

ABSTRACT Magnetic cataclysmic variables of the intermediate polar (IP) subclass display a wide range of variability across different wavelengths. In late 2024 October/early November, the IP V709 Cas was observed over 10 nights by the OPtical TIming CAMera at the San Pedro Mártir Observatory in simultaneous three-colour (g, r, and i, or z band) photometry. On two of these nights, V709 Cas was simultaneously observed by the Neutron star Interior Composition ExploreR X-ray telescope. A periodogram analysis of the optical g- and r-band light curves reveals no prominent features at the white dwarf (WD) spin, but prominent features at the spin-orbit beat. In contrast, the X-ray and near-infrared (near-IR) i- and z-band periodograms show prominent features at the spin, but not the spin-orbit beat. Optical beat and near-IR spin pulsations have been seen in the IP PQ Gem, with simultaneous circular polarization detected in the near-IR, indicating cyclotron origin. We therefore speculate that we are seeing cyclotron radiation from V709 Cas, possibly adding it to the small group of cyclotron-emitting IPs. Combining analytical approximations with our expectation for cyclotron harmonics in the near-IR, we suggest a WD magnetic field strength of $10~{\rm MG} < B < 40$ MG.

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Publication Details

Journal
Monthly Notices of the Royal Astronomical Society
Published
2025-12-08
DOI
https://doi.org/10.1093/mnras/staf2177
Primary Topic
Astrophysical Phenomena and Observations
Type
article
Field-Weighted Citation Impact
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article

OPTICAM reveals hints of cyclotron emission from the intermediate polar V709 Cas

F. Vincentelli, R. Michel, Noel Castro Segura, A. Castro et al.
Monthly Notices of the Royal Astronomical Society
Astrophysical Phenomena and Observations
article

OPTICAM reveals hints of cyclotron emission from the intermediate polar V709 Cas

F. Vincentelli, R. Michel, Noel Castro Segura, A. Castro, Domitilla de Martino, Z A Irving, Simone Scaringi, D. A. H. Buckley, D. Altamirano, M Veresvarska
article en

Abstract

ABSTRACT Magnetic cataclysmic variables of the intermediate polar (IP) subclass display a wide range of variability across different wavelengths. In late 2024 October/early November, the IP V709 Cas was observed over 10 nights by the OPtical TIming CAMera at the San Pedro Mártir Observatory in simultaneous three-colour (g, r, and i, or z band) photometry. On two of these nights, V709 Cas was simultaneously observed by the Neutron star Interior Composition ExploreR X-ray telescope. A periodogram analysis of the optical g- and r-band light curves reveals no prominent features at the white dwarf (WD) spin, but prominent features at the spin-orbit beat. In contrast, the X-ray and near-infrared (near-IR) i- and z-band periodograms show prominent features at the spin, but not the spin-orbit beat. Optical beat and near-IR spin pulsations have been seen in the IP PQ Gem, with simultaneous circular polarization detected in the near-IR, indicating cyclotron origin. We therefore speculate that we are seeing cyclotron radiation from V709 Cas, possibly adding it to the small group of cyclotron-emitting IPs. Combining analytical approximations with our expectation for cyclotron harmonics in the near-IR, we suggest a WD magnetic field strength of $10~{\rm MG} < B < 40$ MG.

Monthly Notices of the Royal Astronomical SocietyVol. 545(3)
University of Cape Town (ZA), Universidad Autónoma de Baja California (MX), Durham University (GB), Astronomical Observatory of Capodimonte (IT), Ensenada Institute of Technology (MX), University of Warwick (GB), Institute for Space Astrophysics and Planetology (IT), South African Radio Astronomy Observatory (ZA), Astronomical Observatory (RS), University of Southampton (GB)
Smithsonian Institution, National Aeronautics and Space Administration, UK Research and Innovation, Ministerio de Ciencia, Innovación y Universidades, European Commission, Goddard Space Flight Center, Smithsonian Astrophysical Observatory, HORIZON EUROPE Framework Programme, Science and Technology Facilities Council, Agencia Estatal de Investigación, Astrophysics Science Division, Astrophysics Division
Openalex Percentile: Top 73%
Astrophysical Phenomena and Observations
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