A flash of X-ray light has revealed the existence of an odd couple of stars, a massive star and a white dwarf, that shouldn't really exist together.
When they reach the end of their long evolutions, smaller stars—those up to eight times as massive as our own sun—typically become white dwarfs. These ancient stars are incredibly dense.
Recent observations of white dwarf explosions have revealed new insights into their diversity and relationship to dark energy ...
The light output of exploding white dwarf stars, which are the stellar corpses of stars with masses around that of the sun, is so uniform that astronomers can use it to measure distances.
Astronomers used a 3D global computer model to compare the climates of exoplanets in different stellar and orbital configurations. They found that a planet orbiting a white dwarf star would offer a ...
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