Image Details

Choose export citation format:

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 A3.

Güdel–Benz diagram including ASKAP J181335−604720 and other M dwarfs. The red star marks ASKAP J181335−604720, while the blue circles, black squares, and black stars denote literature M dwarfs, activity-driven candidates, and auroral candidates from B. J. S. Pope et al. (2021), respectively. The green solid line shows the canonical Güdel–Benz relation, LX/LR = 1015.5 Hz, and the shaded region indicates the ±0.5 dex scatter (M. Guedel & A. O. Benz 1993; A. O. Benz & M. Guedel 1994).

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse