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How is the market cap and valuation of EPL Limited (500135) ✌️【Self-Scheduling】✌️ Expert predictions with real-time stock, futures, and metals, energy data to help you quickly recover and grow. When a supernova was seen glittering in the night sky for six months in 1181, it was so bright that Chinese and Japanese astronomers recorded it as a “guest star” in the Cassiopeia constellation.
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It’s the first time the wispy strands, resembling a dandelion flower, have been observed in 3D as they stream away from the blast site around the dead star. The researchers shared the results of their work, which provide new clarity about the structure of the supernova remnant, in a paper published October 24 inThe Astrophysical Journal Letters.
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“A standard image of the supernova remnant would be like a static photo of a fireworks display,” said study coauthor Christopher Martin, professor of physics at the California Institute of Technology and lead for the team that built the imager, in a statement.“KCWI gives us something more like a ‘movie’ since we can measure the motion of the explosion’s embers as they streak outward from the central explosion.”
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Patchick spotted a nebula near the original site of the supernova while sifting through images taken by NASA’s now-retired Wide-field Infrared Survey Explorer mission. Albert Zijlstra, a professor of astrophysics at the University of Manchester in England, later madethe connection between the nebula and SN 1181in 2021.
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“Because this was a failed explosion, it was fainter than normal supernovae, which has been shown to be consistent with the historical records,” said colead study author Ilaria Caiazzo, assistant professor at the Institute of Science and Technology Austria, in a statement.
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It’s similar to the Doppler effect observed when emergency vehicles turn on their sirens; the horn of an approaching vehicle will emit a higher frequency, but as it moves away, the sound waves stretch out and release a lower frequency.
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“We find the material in the filaments is expanding ballistically,” said colead study author Tim Cunningham, a NASA Hubble Fellow at the Center for Astrophysics | Harvard & Smithsonian, in a statement. “This means that the material has not been slowed down nor sped up since the explosion. From the measured velocities, looking back in time, you can pinpoint the explosion to almost exactly the year 1181.”
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“There are two proposed scenarios: 1) a shock wave moving back towards the star is sublimating dust into hot gas, which then rapidly cools and coalesces into straight filaments or 2) clumps of dust are being stripped by the fast wind of the central star,” Cunningham said in an email. “Our observations are not able to distinguish between these two models, and more observations and theory are needed to understand this nebula, but our observations provided an important piece of the puzzle!”
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Ko was not involved in the new Keck Cosmic Web Imager observations, but he and his colleaguespublished a studyearlier this year suggesting that the supernova remnant is composed of multiple regions, making it difficult to reconcile the exact composition of the filaments.
How is the market cap and valuation of EPL Limited (500135) ✌️【Self-Scheduling】✌️ Real-time stock and futures data, backed by expert stock market trend predictions, to help you make timely and profitable investment decisions. The observations from the new study show that the filaments only extend across the outer regions of the nebula, rather than from the center outward, Ko said, which adds further evidence to the idea that multiple regions are within the supernova remnant. And the more clarity researchers have about the structure of the filaments, the more likely they are to uncover what formed the cosmic dandelion in the first place.
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