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S Doradus (also known as S Dor) is one of the brightest stars in the Large Magellanic Cloud (LMC), a satellite galaxy of the Milky Way, located roughly 160,000 light-years away. The star is a luminous blue variable , and one of the most luminous stars known , having a luminosity varying widely above and below 1,000,000 times the luminosity of ...
15 Ιουν 2022 · While using the Atacama Large Millimeter/submillimeter Array (ALMA) to observe large star-forming regions in the Large Magellanic Cloud (LMC), scientists discovered a turbulent push-and-pull dynamic in the star-forming region, 30 Doradus.
An S Doradus star is a massive, blue supergiant variable star, also known as a Hubble-Sandage variable or a luminous blue variable. S Doradus stars are the most luminous stars in the Galaxy and are easily identified in other nearby galaxies, including the Andromeda Galaxy and the Triangulum Galaxy .
16 Απρ 2012 · Several million young stars are vying for attention in a new NASA Hubble Space Telescope image of a raucous stellar breeding ground in 30 Doradus, a star-forming complex located in the heart of the Tarantula nebula.
10 Ιαν 2023 · The chemical composition of 30 Doradus is different from most of the nebulas found in the Milky Way. Instead it represents the conditions in our galaxy that existed several billion years ago when stars were forming at a much faster pace than astronomers see today.
26 Ιουλ 2001 · This fertile star-forming region, called the 30 Doradus Nebula, has a sparkling stellar centerpiece: the most spectacular cluster of massive stars in our cosmic neighborhood of about 25 galaxies.
23 Ιουλ 2019 · At the center of 30 Doradus, one of the largest star-forming regions located close to the Milky Way, thousands of massive stars are blowing off material and producing intense radiation along with powerful winds.
