A NICER View of a Bursting X-ray Binary
Researchers analyze 51 X-ray bursts from a neutron star snaring material from its stellar companion, forming one of the most active low-mass X-ray binaries known.
Researchers analyze 51 X-ray bursts from a neutron star snaring material from its stellar companion, forming one of the most active low-mass X-ray binaries known.
In 2021, astronomers saw a star explode, then watched as its remains strangely changed colors. A recent study suggests an explanation for this behavior: the remnants hit a speed bump.
Does a massive explosion of solar plasma — a coronal mass ejection — move through the solar system differently if other explosions preceded it?
Deducing the mass of the gas in a protoplanetary disk is notoriously tricky. In this study, a team develops and deploys a new technique to tackle the challenge.
Researchers test an instrument’s ability to detect a certain class of biosignature molecules, potentially providing a way to detect life in the hidden oceans of icy solar system moons.
What’s the latest in the field of supernova research? Five recent articles tackle different aspects of these exploding stars.
Astronomers speculate on the origins of water emission lines in the spectrum of VV Corona Australis A.
When supermassive black holes gulp down gas, the superheated gas shines across the electromagnetic spectrum. Could the composition of this gas affect the radiation we observe?
The Extreme-ultraviolet Snapshot Imaging Spectrograph (ESIS) may help researchers understand the complex region between the Sun’s lower and upper atmosphere.
The deepest extragalactic data from the JWST Early-Release Science program come into focus in research articles published today in the Astrophysical Journal Letters.