Researchers explore the possibility that similar physical processes are responsible for the intriguing filamentary structures at the center of our galaxy and recently discovered in the space between galaxy clusters.

Combining two algorithms allows researchers to identify the locations of lunar swirls: areas of the Moon’s surface that are slightly more reflective than nearby regions, potentially due to magnetic anomalies.

Extensive radio observations suggest that supernova SN2004C lost mass at a highly variable rate in the time before exploding, potentially due to gravity (not gravitational!) waves or binary interaction.

Researchers demonstrate the first use of Stochastic Speckle Discrimination on an extended source, showing that this technique can distinguish between errant speckles and stellar or planetary companions.

Five galaxies observed by JWST show signs of having high-temperature, low-metallicity gas and intense star formation, and new techniques used to analyze the data may reduce systematic errors.

Radio observations of carbon dioxide allow researchers to trace the distribution of ice in a galaxy with robust star formation, finding that ice is likely sublimated efficiently in this galaxy due to shocks.