Research news on Warm-hot intergalactic medium

The warm-hot intergalactic medium (WHIM) research area investigates the diffuse, highly ionized baryonic component of the cosmic web at temperatures of roughly 10⁵–10⁷ K, believed to host a substantial fraction of the “missing” baryons at low redshift. This field combines cosmological simulations with multiwavelength observations, particularly soft X-ray and far-ultraviolet spectroscopy, to detect weak absorption or emission signatures from ions such as O VI, O VII, and O VIII in filaments between galaxies. Research focuses on WHIM thermodynamics, metal enrichment, shock-heating processes, and its role in structure formation, baryon cycling, and feedback from galaxies and active galactic nuclei.

Life in Space: A beginner's guide to life in the universe

Exploring one of science's most exciting frontiers, the book "Life in Space" bridges astrophysics and biology to uncover the conditions that make life possible—on Earth and beyond. Designed for students and general readers ...

Public takes the lead in discovery of new exploding star

Previously described as playing astronomical "spot the difference," Kilonova Seekers asks the public to compare the latest images of a section of night sky to an image of the same section of space taken on previous nights. ...