An AWSoM Model of the Sun
Solar physicists have simulated conditions in and around a solar active region using a particularly high-resolution model of the Sun’s atmosphere for the first time.
Solar physicists have simulated conditions in and around a solar active region using a particularly high-resolution model of the Sun’s atmosphere for the first time.
What’s the cause of the new X-ray source MAXI J1848-015 that flared into view for only a few days?
What determines whether a planet orbiting two stars does so in the same plane as the binary system, perpendicular to it, or somewhere in between?
What can studying the spins of galaxies and their associated dark matter halos tell us about cosmology?
Astronomers use an array of radio telescopes to search for the galactic neighbors of some of the brightest objects in the universe.
A new focus issue examines the survey strategy for the Vera C. Rubin Observatory’s Legacy Survey of Space and Time.
Astronomers have captured submillimeter pulses from a highly magnetized, city-sized stellar remnant for the first time.
HIP 41378 f’s bulk density is extremely low. Is it a puffy planet, are rocky rings playing a role, or is it something else altogether?
Can we figure out the initial magnetic field configuration of two neutron stars given the magnetic field after they’ve collided?
Only four galaxies in the universe are known to exhibit strange, high-energy eruptions. Now, a serendipitous search may have turned up a fifth.