The Expansion of the Universe on Another Mode
Certain features of the cosmic microwave background could help us measure how quickly the universe is expanding.
Certain features of the cosmic microwave background could help us measure how quickly the universe is expanding.
Models suggest that black holes of a certain mass can’t be produced by supernovae. Gravitational-wave signals from black hole mergers can allow us to test this prediction of “missing” black holes.
Scientists have explored how delicate filaments of cold gas form and survive within the hot, fast-moving surroundings of an active galaxy.
New observations of a massive neutron star provide clues about these extreme objects’ interiors.
How can we spot supermassive black holes lurking outside of their galaxies’ centers? These wanderers may not remain lost!
What does the afterglow of a binary neutron star merger look like? Simulations can give us a fairly good approximation.
The disk of the Milky Way glows in high-energy gamma-ray photons — but where does this diffuse emission come from?
New images reveal the role played by whirling magnetic fields in the shrouded centers of clouds forming baby massive stars.
Scientists are using a powerful telescope to hunt for planets in our nearest star system, Alpha Centauri AB.
With data from the Gaia satellite and spectroscopic surveys, machine learning can fill in gaps in our knowledge of how stars move.