Distant Little Red Dot Hosts a Huge (and Growing) Black Hole
The “little red dot” CAPERS-LRD-z9 is the most distant object to show the characteristic broad emission lines of fast-moving gas around a black hole.
The “little red dot” CAPERS-LRD-z9 is the most distant object to show the characteristic broad emission lines of fast-moving gas around a black hole.
New observations from the X-Ray Imaging and Spectroscopy Mission (XRISM) show the multilayered winds of NGC 4151 in a whole new light.
Worth the wait: using observations separated by 15 years, researchers have clocked the speed of a neutron star flying through space and shed light on how these stellar remnants are launched by supernova explosions.
Catch up on recent astronomy news: a stellar navigation experiment, a doomed planet, an icy protostar, and a mysterious radio source.
The dust in protoplanetary disks is subject to complicated dynamical processes that impact planet formation. Recent simulations suggest that dust may be more freely moving within disks with planets than previously thought.
Finally found: using speckle imaging, researchers have spotted what is likely the predicted 1.6-solar-mass companion to the red supergiant Betelgeuse.
What’s responsible for the haphazard orbits of the stars closest to our galaxy’s supermassive black hole? A second black hole, perhaps.
One of the first-look images from the Vera C. Rubin Observatory contained a rare find: a candidate circumstellar or protoplanetary disk in a region where few such disks have been discovered.
A search for oddities in archival JWST data has turned up something remarkable: a rare pair of collisional ring galaxies that may have birthed a supermassive black hole during their clash.
A recently discovered tidal disruption event has astronomers investigating new ways in which stars may be ripped apart by supermassive black holes.