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Low, Low, and Lower: A Binary Ultracool Dwarf System is Detected at 340 MHz

The lowest mass stars have been well-studied across the mid and high frequency radio bands. However, lower frequencies can reveal larger-scale magnetic structures and may even be the key to the first direct radio detection of an exoplanet. Learn about the first detection of a low-mass ultracool dwarf–one or both stars in a binary system–at the low frequency of 340 MHz!

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