File:Neutron star merger and cocoon Kasliwal 2017.ogv
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Summary[edit]
DescriptionNeutron star merger and cocoon Kasliwal 2017.ogv |
English: A hydrodynamical simulation shows a cocoon breaking out of the neutron star merger. This model explains the gamma-ray, X-ray, ultraviolet, optical, infrared, and radio data gathered by the GROWTH team from 18 telescopes around the world. |
Date | |
Source |
Movie S1 from the SUPPLEMENTARY MATERIALS from paper "Illuminating gravitational waves: A concordant picture of photons from a neutron star merger" www.sciencemag.org/cgi/content/full/science.aap9455/DC1 |
Author | Ehud Nakar (Tel Aviv), Ore Gottlieb (Tel Aviv), Leo Singer (NASA), Mansi Kasliwal (Caltech), and the GROWTH collaboration |
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current | 23:46, 30 November 2017 | 5.4 s, 1,424 × 936 (714 KB) | ActiveDendrite (talk | contribs) | User created page with UploadWizard |
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