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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 1.

Simultaneous ASKAP radio and TESS optical observations of ASKAP J181335−604720. Top panel: the TESS relative optical light curve during the ASKAP observing interval, with the flux normalized to the median value and expressed in fractional units. Middle panel: ASKAP radio light curves in Stokes I (black) and Stokes V (red), binned to 60 s for clarity. Bottom panel: dynamic spectrum of the ASKAP Stokes V radio emission, binned to 5 min in time and 8 MHz in frequency for clarity. The gray shaded regions indicate the epochs at which radio pulses are detected.

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