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.

The Sun may not engulf Earth after all, scientists say

Need some good news on a Friday after a long week? The Earth may not be engulfed by the expanding fireball of the dying sun, which has long been assumed to be our home planet's ultimate fate, according to scientists.

A star's death throes involve a lot of kicking

When stars like our sun age, they puff up into red giants. Their bubbling outer mass gradually escapes into space, and their remaining cores contract into white dwarfs. Since most stars end their lives this way, the universe ...

First outbursting hot subdwarf binary discovered

An international team of astronomers has utilized the Zwicky Transient Facility (ZTF) and the Transiting Exoplanet Survey Satellite (TESS) to investigate a binary system designated ZTF J0007+4804. As a result, they have found ...

One graph attempts to connect every object in the universe

If you've ever taken an introductory astronomy class, you've probably seen the Hertzsprung-Russell (HR) diagram. This graph maps out the life cycle of stars by plotting their temperature against their luminosity, and has ...

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