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<oembed><version>1.0</version><provider_name>KMI - Nagoya University</provider_name><provider_url>https://www.kmi.nagoya-u.ac.jp/eng</provider_url><title>Multi-Messenger Era of High Energy Astrophysics - KMI - Nagoya University</title><type>rich</type><width>600</width><height>338</height><html>&lt;blockquote class="wp-embedded-content" data-secret="JarKy9DI6Q"&gt;&lt;a href="https://www.kmi.nagoya-u.ac.jp/eng/seminar/999/"&gt;Multi-Messenger Era of High Energy Astrophysics&lt;/a&gt;&lt;/blockquote&gt;&lt;iframe sandbox="allow-scripts" security="restricted" src="https://www.kmi.nagoya-u.ac.jp/eng/seminar/999/embed/#?secret=JarKy9DI6Q" width="600" height="338" title="&#x201C;Multi-Messenger Era of High Energy Astrophysics&#x201D; &#x2014; KMI - Nagoya University" data-secret="JarKy9DI6Q" frameborder="0" marginwidth="0" marginheight="0" scrolling="no" class="wp-embedded-content"&gt;&lt;/iframe&gt;&lt;script type="text/javascript"&gt;
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</html><description>High energy phenomena, such as gamma-ray bursts and cosmic rays, are ubiquitous in the universe. Revealing their origin and evolution is one of the most interesting subjects in the studies of the universe. Deeply understanding these phenomena also provides feedback on cosmology as well as high-energy and high-density physics. The last decades witnessed the great progress in this field. We have now established that stellar collapses produce supernova explosions and sometimes gamma-ray bursts. Stellar explosions release heavy elements into space, &hellip;</description></oembed>
