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Rotationally Modulated Highly Circularly Polarized Radio Pulses from the Rapidly Rotating M Dwarf ASKAP J181335−604720

  • Authors: Shouzhi Wang, 守智 王, Biwei Jiang, 碧沩 姜, Qichen Huang, 启宸 黄, Shaoteng Huang, 少腾 黄, Jundan Nie, 俊丹 聂

Shouzhi Wang et al 2026 The Astrophysical Journal Letters 1003 .

  • Provider: AAS Journals

Caption: Figure 3.

Phase-folded ASKAP radio light curves from two observing epochs. The ASKAP Stokes I (black) and Stokes V (red) time series are phase-folded using the optical rotation period P = 5.607 hr derived from the TESS photometry, with the start time of ASKAP Epoch 1 adopted as the reference phase zero-point. The top and bottom panels show Epoch 1 and Epoch 2, respectively.

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