A Contracting White Dwarf?
A peculiar X-ray binary may contain the first known white dwarf which is still in the process of contracting.
A peculiar X-ray binary may contain the first known white dwarf which is still in the process of contracting.
40 Eridani B was the first white dwarf to be discovered, but details of its structure and composition remained a mystery, until today’s paper.
Pulsations are the way for astronomers to probe the interior of stars. Today’s paper announces the discovery of a new class of pulsator stars. What makes them different? And what exciting new things can we learn from that?
Image credits: Paweł Pietrukowicz
The accuracy of our estimates of the radii of white dwarf stars has important implications to cosmology. We currently rely on a theoretical mass-radius relationship for that. Are we doing a good job?
Image credits: RJHall/Wikimedia Commons.
The discovery of carbon-rich Mira variables in the Galactic centre could imply the existence of a number of young stars among the otherwise old Galactic bulge population.
Stellar evolution remains one of the most complicated and yet fundamental subjects in astrophysics. In today’s paper, we take a look at the role of atomic diffusion in the evolution of Sun-like stars, and how they affect estimates of stellar ages and chemical tagging.