Constraining the Emission Geometry and Mass of the White Dwarf Pulsar AR Sco Using the Rotating Vector Model
Author:
Funder
National Research Foundation
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/1538-4357/ab4e19/pdf
Reference31 articles.
1. The spin axes orbital alignment of both stars within the eclipsing binary system V1143 Cyg using the Rossiter-McLaughlin effect
2. Gravitational two-body problem with arbitrary masses, spins, and quadrupole moments
3. Relativistic effects in the binary pulsar PSR 1913+16
4. Polarimetric evidence of a white dwarf pulsar in the binary system AR Scorpii
5. Polarization of the binary radio pulsar 1913 + 16 - Constraints on geodetic precession
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2. VLBI astrometry on the white dwarf pulsar AR Scorpii;Monthly Notices of the Royal Astronomical Society;2023-01-30
3. Evidence for an abundant old population of Galactic ultra-long period magnetars and implications for fast radio bursts;Monthly Notices of the Royal Astronomical Society;2023-01-20
4. Spun-Up Rotation-Powered Magnetized White Dwarfs in Close Binaries as Possible Gamma-ray Sources: Signatures of Pulsed Modulation from AE Aquarii and AR Scorpii in Fermi-LAT Data;Galaxies;2023-01-11
5. Long-term photometric monitoring and spectroscopy of the white dwarf pulsar AR Scorpii;Monthly Notices of the Royal Astronomical Society;2022-08-26
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