First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir

arXiv:2608.00968 · astro-ph.SR · Submitted 2026-08-02 · Read on arXiv

Barnali Das, Hayley Bignall, Andrew Zic, Poonam Chandra, Joshua Pritchard, John Morgan, Ankita Ghosh, Bhaswati Bhattacharyya, George Hobbs

astro-ph.SR

Submitted: 2026-08-02

Comments: Accepted for publication in ApJ

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Frequency Dependence — 2× in this paper · explained in 2 episodes
• Calibration — 1× in this paper · explained in 7 episodes
• Trace — 1× in this paper · explained in 2 episodes
• Very Large Array — 1× in this paper

Sources

• Coherent radio emission from 'Main-sequence Radio Pulse emitters': a new stellar diagnostic to probe 3D magnetospheric structures
• Probing the magnetospheres of hot magnetic stars using ECME
• Towards comprehension of the variability of the magnetic chemically peculiar star CU Virginis (HD 124224)
• A retrospective view of Miriad
• Coherent radio emission from the magnetic chemically peculiar star CU Virginis

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