Page 3: 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 examines 'Exposed Cranium' nebula

Two heads are better than one in the latest images from NASA's James Webb Space Telescope, which reveal new detail in a mysterious, little-studied nebula surrounding a dying star. Nebula PMR 1 is a cloud of gas and dust that ...

Image: Artist's concept of a white dwarf star

A smaller white dwarf star (left) pulls material from a larger star into a swirling accretion disk in this artist's concept released Nov. 19, 2025, to illustrate the first use of NASA's IXPE (Imaging X-ray Polarization Explorer) ...

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