U.Scorpii: This 3D simulation, from a paper by Drake & Orlando, explores the first 18 hours after the last outburst observed by the nova system in 2010. Astronomers have seen U Scorpii erupt about once every decade, so this system is due for another outburst very soon.pic.twitter.com/UOabWoGQJ2
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Cas A: By modeling this supernova remnant in 3D, S.Orlando et al show the massive clumps that developed soon after the star's explosion are likely responsible for the asymmetrical shape of Cas A.pic.twitter.com/rjexy6IEDm
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DG Tau: Stellar jets, detected in X-rays by Chandra, generate shock waves similar to those produced by supersonic jets. A paper led by S.Ustamujic compares their 3D computer models w/data from 2 young stars observed with Chandra.pic.twitter.com/xoDCgCwIjX
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SN 1006: This 3D model, from a paper by S.Orlando et al, shows the remnant that resulted from the explosion & destruction of a white dwarf star. The model helps explore how the clumping of material & the acceleration of high-energy particles affects the structure of the remnant.pic.twitter.com/vWQ4Q8e0w0
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SN 1987a: The supernova's expanding remnant offers the opportunity to unveil the physical processes associated with the supernova & the final stages of stellar evolution. This model from Orlando et al shows the remnant in 2017pic.twitter.com/BTwHqXsmsx
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thanks, the link is the last thread in the tweet. are you able to see it?https://twitter.com/kimberlykowal/status/1222566560570707968?s=20 …
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Wonderful! Imagination travels faster than light.
Hvala. Twitter će to iskoristiti za poboljšanje vaše vremenske crte. PoništiPoništi
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Čini se da učitavanje traje već neko vrijeme.
Twitter je možda preopterećen ili ima kratkotrajnih poteškoća u radu. Pokušajte ponovno ili potražite dodatne informacije u odjeljku Status Twittera.