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!
Today’s astrobite looks at how we can use observations of gamma-rays and neutrinos to test our models of cosmic rays.
JWST offers new insights into the vertical structure of this protoplanetary disc, special for the ambient emitting background that provides a back-light. Find out what the JEDIce program has discovered!
Subtle whispers in gravitational waves put general relativity to the test.
Today’s paper argues that a little red dot with a massive Balmer break could be a black hole star.
Simulating an entire galaxy is not easy if you want your result sometime this century. But today’s paper brings us a neat trick that might just help speed things up.