News
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Space.com on MSNAstronomers trace mysterious blast of X-rays to 'Die Hard' star that refuses to perish (video)"This discovery heralds a broader understanding of the diversity in massive stars' deaths and a need for deeper investigations into the whole landscape of stellar evolution." ...
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Study Finds on MSN‘Dark Dwarfs’ Might Be Glowing In The Milky Way, Powered By Dark MatterNew research suggests sub-stellar objects called dark dwarfs could glow forever on dark matter energy. Could they reveal secrets about the universe’s hidden mass?
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ScienceAlert on MSNDying Star's Strangled Jets Solve 50-Year-Old X-Ray MysteryA new study of a star undergoing the throes of a supernova death has revealed that bursts of X-radiation known as fast-X-ray ...
Very massive stars are cosmic "rock stars" that live fast, die young and leave black holes in their place. During this ...
Using a combination of telescopes, astronomers have characterized the closest supernova linked to a fast X-ray transient. The ...
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Space.com on MSNHubble Telescope finds stellar nursery in Taurus Molecular Cloud | Space photo of the day for July 2, 2025The Hubble Space Telescope searches the universe to understand how planets, stars, and galaxies form. Recently, it captured ...
Researchers from the Xinjiang Astronomical Observatory (XAO) of the Chinese Academy of Sciences have made significant ...
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Futurism on MSNAstronomers Capture First-Ever Image of Star That Exploded TwiceAstronomers have taken the first ever image that shows what happens when a star explodes twice in a supernova.
Triple Star Systems: A Key to Understanding Stellar Evolution. Triple star systems, though accounting for about 10% of Sun-like stars, remain poorly understood.
Astronomers have discovered a new star that is 30 times larger than the sun and could force a major rethink of stellar evolution theories. The star, designated J0524-0336 and located around 30,000 ...
Astrophysics: Star-childhood shapes stellar evolution Date: September 19, 2022 Source: University of Innsbruck Summary: In classical models of stellar evolution, so far little importance ...
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