SDSS astronomers observe theoretically predicted effect in the remnants of dead stars
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SDSS astronomers observe theoretically predicted effect in the remnants of dead stars

A student-led team has observed that the mass-radius relation of white dwarf stars, a type of star which is so dense that they are supported by quantum mechanical effects, depends on the temperature of the star. Scientists have long searched for this subtle effect, detected here for the first time using a method from General Relativity – along with the largest catalog of white dwarf data of its kind.

The “Barbenheimer Star”: Evidence for Spectacular Nucleosynthesis in the Early Universe
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The “Barbenheimer Star”: Evidence for Spectacular Nucleosynthesis in the Early Universe

Astronomy’s new blockbuster is now playing in New Orleans. Astronomers from the Sloan Digital Sky Survey (SDSS) have discovered evidence for what they call the “Barbenheimer Star” – an enormous ancient star that exploded in a way previously thought impossible, resulting in an unusual pattern of elemental ashes that left behind a trail of evidence still visible billions of years later.

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