Rapidly rotating magnetic star HR 5907 emits unusual low-frequency radio signals

23. 1. 2025

Rapidly rotating magnetic star HR 5907 emits unusual low-frequency radio signals

Star system: HR 5907 | Distance from the Sun: 467 light years

Its circular polarization suggests persistent auroral activity via electron cyclotron maser emission

Generated by LLM, corrected by human

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Stars Massive main-sequence stars

Scientific study

A Non-Stop Aurora? The Intriguing Radio Emission from the Rapidly Rotating Magnetic Massive Star HR 5907 external link

Stars mentioned

HR 5907

B2.5V, Blue-white star

mass: 5.5 M☉

radius: 4 R☉

distance: 467 ly

stars in the system: 1

exoplanets: 0

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