{"id":4544,"date":"2019-09-08T16:33:39","date_gmt":"2019-09-08T14:33:39","guid":{"rendered":"https:\/\/www.oa-cagliari.inaf.it\/seminari\/perche-studiare-le-nebulose-a-vento-di-pulsar\/"},"modified":"2025-09-22T23:01:04","modified_gmt":"2025-09-22T21:01:04","slug":"perche-studiare-le-nebulose-a-vento-di-pulsar","status":"publish","type":"seminari","link":"https:\/\/www.oa-cagliari.inaf.it\/en\/seminars\/perche-studiare-le-nebulose-a-vento-di-pulsar\/","title":{"rendered":"Why Study Pulsar Wind Nebulae?"},"content":{"rendered":"

\"\"<\/p>\n

The majority of core collapse supernova are believed to produce a neutron star, whose rotational energy powers an extremely relativistic pulsar wind whose interaction with the surroundings creates a pulsar wind nebula. In this talk, I will demonstrate how pulsar wind nebula can be used to study a wide range of high-energy phenomena: from the physics of core-collapse supenovae to the creation and acceleration of extremely high energy leptons.<\/p>\n","protected":false},"template":"","class_list":["post-4544","seminari","type-seminari","status-publish","hentry","categorie_seminari-colloquium"],"acf":[],"_links":{"self":[{"href":"https:\/\/www.oa-cagliari.inaf.it\/en\/wp-json\/wp\/v2\/seminari\/4544","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.oa-cagliari.inaf.it\/en\/wp-json\/wp\/v2\/seminari"}],"about":[{"href":"https:\/\/www.oa-cagliari.inaf.it\/en\/wp-json\/wp\/v2\/types\/seminari"}],"wp:attachment":[{"href":"https:\/\/www.oa-cagliari.inaf.it\/en\/wp-json\/wp\/v2\/media?parent=4544"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}