Page 2: Research news on Interstellar magnetic fields

Interstellar magnetic fields as a research area focuses on the origin, structure, strength, and evolution of magnetic fields in the diffuse and dense phases of the interstellar medium (ISM) of galaxies. It integrates observational probes (e.g., Faraday rotation, Zeeman splitting, synchrotron emission, dust polarization) with magnetohydrodynamic (MHD) theory and simulations to understand how magnetic fields influence star formation, cosmic-ray propagation, ISM turbulence, and galactic dynamos. The field also investigates magnetic coupling between different ISM phases, feedback from stellar winds and supernovae on field topology, and the role of magnetization in shaping filaments, molecular clouds, and large-scale galactic structures.

Preparing for the greatest cosmic movie ever made

High up on the top of Cerro Pachón in northern Chile, NSF–DOE Vera C. Rubin Observatory is nearing completion. At the heart of the facility, a pivotal moment in the project's scientific adventure is unfolding. After more ...

Signs of alien life may be hiding in these gases

Scientists have identified a promising new way to detect life on faraway planets, hinging on worlds that look nothing like Earth and gases rarely considered in the search for extraterrestrials.

A new way to detect daisy worlds

The daisy world model describes a hypothetical planet that self-regulates, maintaining a delicate balance involving its biogeochemical cycles, climate, and feedback loops that keep it habitable. It's associated with the Gaia ...

page 2 from 2