Metal Before It Was Cool: Super-Enrichment in the Early Universe
Galaxies in the early universe were mostly pure hydrogen. How, then, did one end up with so much metal just a billion years after the Big Bang?
Galaxies in the early universe were mostly pure hydrogen. How, then, did one end up with so much metal just a billion years after the Big Bang?
If dark matter and normal matter could interact, it could ease the emerging tension between measurements of how smooth or clumpy the distribution of matter is in our universe.
Machine learning is increasingly popular in many fields of science, including astrophysics. Today’s post takes a look at how machine-learning techniques have been used in three research areas.
The gravitational waves emitted by stellar-mass black holes merging with one member of a supermassive black hole binary might be a prominent target for upcoming observatories like LISA.
The New Horizons spacecraft flew by the Kuiper Belt object Arrokoth more than four years ago. Today, this fascinating, lumpy, bi-lobed object still holds plenty of mysteries.
SN 2023ixf, which was discovered in May 2023 in the Pinwheel Galaxy, is the nearest extragalactic supernova observed in almost a decade. What did early data tell us about the event?
If you wanted to know what’s in the air of a lava planet, it wouldn’t be a good idea to go visit in person. Luckily, astronomers don’t have to.
Researchers take a wide view of an unusual repeating fast radio burst to decode the burst’s dispersed signal.
Why did a small galaxy stop forming stars less than 700 million years after the Big Bang? Cosmological simulations give some clues about why star formation stalled.
Quiescent elliptical galaxies might harbor a new class of rare transients called luminous fast coolers, the physical origins of which remain unknown.