Classic theory says only big clouds should survive galactic winds, but these new simulations show that’s not the whole story. Whether a cloud lives or dies depends not only on its size, but also on the environment it’s sitting in.
How is the growth of massive black holes regulated by starlight and stellar explosions? Learn more in today’s bite!
Today’s authors use FLAMINGO simulations to probe the tension between different observational methods of estimating cosmological parameters.
Turns out there’s more than one way to “plate” a planet!
Today’s authors consider the way AGN jet shape changes our measurements of blazar polarization.
When we don’t have spectra, we can estimate the distance to a quasar by calculating its photometric redshift. Today’s authors present a new way to use the ‘flickering’ of quasars to improve these distance estimates.