Statistical analysis of radio-flaring brown dwarf population
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Statistical analysis of radio-flaring brown dwarf population

Brown dwarfs are known as “failed stars,” owing to the lack of central hydrogen burning. They bridge the gap between planets and stars. Some brown dwarfs are found to maintain kilogauss magnetic fields and produce flaring radio emissions, similar to aurora on magnetized planets in solar system, arousing astronomers’ curiosities about their field properties and dynamics.

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