{"id":712,"date":"2023-02-17T11:50:49","date_gmt":"2023-02-17T03:50:49","guid":{"rendered":"https:\/\/www.astro.ncu.edu.tw\/taova\/?page_id=712"},"modified":"2023-11-02T14:24:58","modified_gmt":"2023-11-02T06:24:58","slug":"2023ssp-7","status":"publish","type":"page","link":"https:\/\/www.astro.ncu.edu.tw\/taova\/index.php\/2023ssp-7\/","title":{"rendered":"2023 #14"},"content":{"rendered":"\n<p class=\"has-text-align-center\" style=\"font-size:25px\"><strong>High-energy Observations of Gamma-ray Binaries<\/strong><\/p>\n\n\n\n<p class=\"has-text-align-center has-text-color has-medium-font-size\" style=\"color:#1613f2\">Kwan-Lok Li (Department of Physics, National Cheng Kung University)<\/p>\n\n\n\n<p style=\"font-size:15px\"><br>Gamma-ray binaries are High-Mass X-ray Binaries (HMXBs), which are composed of a massive star and a compact object (neutron star\/pulsar, in most of the cases). These objects show periodic modulated X-rays and gamma-rays through the interaction between the pulsar winds and the stellar winds, although the details are not fully known yet. In this project, we will make use of X-ray observations from Swift, XMM-Newton, and\/or Chandra to study some newly identified gamma-ray binaries.<\/p>\n\n\n\n<p style=\"font-size:15px\">Required Background:<br>Unix\/Linux experience, and Passion.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>High-energy Observations of Gamma-ray Binaries Kwan-Lok &hellip; <a href=\"https:\/\/www.astro.ncu.edu.tw\/taova\/index.php\/2023ssp-7\/\" class=\"more-link\">\u95b1\u8b80\u5168\u6587 <span class=\"screen-reader-text\">2023 #14<\/span><\/a><\/p>\n","protected":false},"author":1,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"ngg_post_thumbnail":0,"footnotes":""},"class_list":["post-712","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/www.astro.ncu.edu.tw\/taova\/index.php\/wp-json\/wp\/v2\/pages\/712","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.astro.ncu.edu.tw\/taova\/index.php\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/www.astro.ncu.edu.tw\/taova\/index.php\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/www.astro.ncu.edu.tw\/taova\/index.php\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/www.astro.ncu.edu.tw\/taova\/index.php\/wp-json\/wp\/v2\/comments?post=712"}],"version-history":[{"count":3,"href":"https:\/\/www.astro.ncu.edu.tw\/taova\/index.php\/wp-json\/wp\/v2\/pages\/712\/revisions"}],"predecessor-version":[{"id":1963,"href":"https:\/\/www.astro.ncu.edu.tw\/taova\/index.php\/wp-json\/wp\/v2\/pages\/712\/revisions\/1963"}],"wp:attachment":[{"href":"https:\/\/www.astro.ncu.edu.tw\/taova\/index.php\/wp-json\/wp\/v2\/media?parent=712"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}