Research news on White dwarf stars

White dwarf stars as a research area encompasses the theoretical and observational study of compact stellar remnants supported by electron degeneracy pressure, focusing on their internal structure, composition (e.g., CO, ONe, or He cores), cooling sequences, and role in stellar and galactic evolution. Research investigates their mass–radius relations, crystallization and phase separation in dense plasmas, atmospheric properties and spectral classification (DA, DB, etc.), and magnetic and rotational characteristics. The field also examines white dwarfs as progenitors of Type Ia supernovae, as laboratories for extreme physics (equations of state, diffusion, convection), and as chronometers for estimating the ages of stellar populations and the Galactic disk.

Webb captures clearest image yet of the Lion Nebula

The NASA/ESA/CSA James Webb Space Telescope recently imaged NGC 2392 (also known as the Lion Nebula), named for its distinctive appearance, which resembles a lion's face seen head-on.

'Dead stars' may have surprisingly healthy appetites

"Dead stars" known as white dwarfs have already shown the potential to help us better understand how planetary systems, including our own solar system, take shape and evolve. Now, research from the University of Michigan ...

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