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Search resuls for: "Takatoshi Ko"


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In this case, filaments radiate away from a “zombie star” the explosion created. Then, in 2023, astronomers spied weird filaments glowing with light from sulfur within the nebula. Scientists know the supernova created the filaments, but it’s unclear how or when the structures formed. The robust data that the instrument captured allowed the team to measure the motions of each filament and create a 3D map. The Keck Cosmic Web Imager enabled measurements of the velocity of any material within the nebula that emits light.
Persons: , Christopher Martin, “ KCWI, Dana Patchick, Patchick, NASA’s, Albert Zijlstra, Ilaria Caiazzo, Tim Cunningham, Zijlstra, Cunningham, ” Cunningham, James Webb, Takatoshi Ko, Ko Organizations: CNN, Keck, California Institute of Technology, Survey, University of Manchester, Pa, Institute of Science, Technology, NASA Hubble, Center, Astrophysics | Harvard & Smithsonian, Southern, Research Center, University of Tokyo Locations: Hawaii, England, Technology Austria
But Zijlstra, who was not involved with the new study, was the first to make the connection to SN 1181. The report suggested that SN 1181 might belong to the elusive Type Iax category of supernova due to the presence of this “zombie” white dwarf. That energy causes the sudden brightness of the supernova.”That massive collision might explain another curious aspect of the SN 1181 zombie star. “We theorize that the star reignited because SN 1181 was a Type Iax supernova, which is an incomplete explosion. Schaefer added that SN 1181 represents one of the few reliable connections from supernova to supernova remnant.
Persons: , Takatoshi Ko, Albert Zijlstra, Dana Patchick, Zijlstra, ” Zijlstra, , coauthors, NASA's Chandra, ” Ko, Chandra, Ko, Bradley Schaefer, Schaefer, ” Schaefer, astrophysicists Organizations: CNN, Astrophysical, University of Tokyo, University of Manchester, Survey, NASA, ESA, JPL, Caltech, Subaru, Louisiana State University Locations: China, Japan, England, New Mexico, Hawaii
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