A reevaluation of the proposed spin-down of the white dwarf pulsar in AR Scorpii
We present high-speed optical photometric observations, spanning ∼2 yr, of the recently discovered white dwarf pulsar AR Scorpii. The amplitudes of the orbital, spin, and beat modulations appear to be remarkably stable and repeatable over the time span of our observations. It has been suggested that...
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| Veröffentlicht in: | Monthly notices of the Royal Astronomical Society. Letters 2018-07, Vol.478 (1), p.L78-L82 |
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| Hauptverfasser: | , |
| Format: | Artikel |
| Sprache: | eng |
| Online-Zugang: | Volltext |
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