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USA-599913-Ret Misc Merchandise Whol Service Establishment Equipme Κατάλογοι Εταιρεία
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Εταιρικά Νέα :
- The models were right: Astronomers find missing matter . . .
Astronomers have discovered a huge filament of hot gas bridging four galaxy clusters At 10 times as massive as our galaxy, the thread could contain some of the universe's 'missing' matter
- Astronomers locate universes missing matter in the largest . . .
"The 'missing' matter may truly be lurking in hard-to-see threads woven across the universe " Astronomers have discovered a vast tendril of hot gas linking four galaxy clusters and stretching out
- Astronomers just found the universes missing matter: Here . . .
Half of ordinary matter in universe has long been 'missing ' Astronomers just found it Revelations made possible by studying radio waves hurtling through space suggest that violent cosmic forces
- Vast Filament of Hidden Matter Seen for the First Time
Cosmological models predict that the missing matter can be found in long filaments that extend between matter densities Astronomers have spotted these filaments, but not with clarity
- Astronomers Uncover a Massive Shaft of Missing Matter
Another clue about the whereabouts of the missing matter in the Universe has just emerged from amid the largest local cosmic structure X-ray observations have revealed a massive filament of hot gas, measuring some 23 million light-years in length, in the space between four sub-clusters of galaxies in the enormous, 8,000-galaxy strong Shapley
- Astronomers Find Universe’s ‘Missing’ Matter, Validating . . .
Cosmic Mystery Solved? Astronomers Find Elusive ‘Missing’ Matter For decades, astronomers have faced a puzzling problem: about a third of the universe’s “normal” matter – the stuff that makes up stars, planets, and galaxies – seemed to be missing Cosmological models predicted its existence, but observations couldn’t find it all
- “The models were right”: astronomers find ‘missing’ matter
Astronomers discover vast filament of ‘missing’ matter Open Image Konstantinos and colleagues characterised the filament by combining X-ray observations from XMM-Newton and Suzaku, and digging into optical data from several others The two X-ray telescopes were ideal partners
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