Tailor-Made Turbulence for All Your Modeling Needs
A new method for modeling turbulent magnetic fields — important for everything from accretion disks to the solar wind — yields realistic fields while also keeping computational costs low.
A new method for modeling turbulent magnetic fields — important for everything from accretion disks to the solar wind — yields realistic fields while also keeping computational costs low.
Supernova hunters have been busy: SN 2024ggi is the second nearby supernova in less than a year. What do archival observations tell us about this supernova’s progenitor star?
Simulations suggest that black holes could have grown to supermassive size with the help of young star clusters in the early universe.
A pair of nearly identical fast radio bursts from different sources gives a hint to the cause of these powerful radio flashes.
Most cool stars spin nicely aligned with their planets. So why do their hot counterparts tumble in nearly random directions?
The supernova SN 2019ein may have originated near a globular cluster — an unusual environment that hints to the nature of the supernova progenitor system.
Meet RX J2129–z8He II: a remarkable high-redshift galaxy that might be home to some of the first generation of stars.
Billions of years ago, small galaxies may have had cores packed with dark matter. What would these galaxies look like today?
A recent study merges different datasets to build a richer picture of Dimorphos, humanity’s first asteroid redirection target.
This month, we’re exploring temperate exoplanets: how to find them, how to model them, and how to figure out if they host life.