Probing the Non-thermal Emission Geometry of AR Sco via Optical Phase-Resolved Polarimetry

Abstract

AR Sco is a binary system that contains a white and red dwarf. The rotation rate of the white dwarf has been observed to slow down, analogous to rotation-powered radio pulsars; it has thus been dubbed a "white dwarf pulsar". We previously fit the traditional radio pulsar rotating vector model to the linearly polarised optical data from this source, constraining the system geometry as well as the white dwarf mass. Using a much more extensive dataset, we now explore the application of the same model to binary phase-resolved optical polarimetric data, thought to be the result of non-thermal synchrotron radiation, and derive the magnetic inclination angle $\alpha$ and the observer angle $\zeta$ at different orbital phases. We obtain a $\sim 10^{\circ }$ variation in $\alpha$ and $\sim 30^{\circ }$ variation in $\zeta$ over the orbital period. The variation patterns in these two parameters is robust, regardless of the binning and epoch of data used. We speculate that the observer is detecting radiation from an asymmetric emission region that is a stable structure over several orbital periods. The success of this simple model lastly implies that the pitch angles of the particles are small and the pulsed, non-thermal emission originates relatively close to the white dwarf surface.

13 pages, 14 figures, accepted by MNRAS

References in corpus (11)

• A radio pulsing white dwarf binary star
• Polarimetric evidence of a white dwarf pulsar in the binary system AR Scorpii
• AR Sco: A White Dwarf Synchronar
• A Model for AR~Scorpii: Emission from Relativistic Electrons Trapped by Closed Magnetic Field Lines of Magnetic White Dwarfs
• Driving the Beat: Time-Resolved Spectra of the White Dwarf Pulsar AR Scorpii
• An Improved Spin-Down Rate for the Proposed White-Dwarf Pulsar AR Scorpii
• Constraining the Emission Geometry and Mass of the White Dwarf Pulsar AR Sco using the Rotating Vector Model
• Peeking Between the Pulses: The Far-UV Spectrum of the Previously Unseen White Dwarf in AR Scorpii
• Magnetospheric interaction in white dwarf binaries AR Sco and AE Aqr
• On the Polarized Nonthermal Emission from AR Scorpii
• ZTF J185139.81+171430.3 = ZTF18abnbzvx: the second white dwarf pulsar?

Cited by in corpus (4)

• Long-term photometric monitoring and spectroscopy of the white dwarf pulsar AR Scorpii
• Cyclotron emitting magnetic white dwarfs in post common envelope binaries discovered with the Zwicky Transient Facility
• VLBI astrometry on the white dwarf pulsar AR Scorpii
• Towards Modelling AR Sco: Generalised Particle Dynamics and Strong Radiation-Reaction Regimes