{"id":17,"date":"2017-10-08T17:25:44","date_gmt":"2017-10-08T15:25:44","guid":{"rendered":"http:\/\/www.issibern.ch\/teams\/blackholebinary\/?page_id=17"},"modified":"2017-10-08T17:25:44","modified_gmt":"2017-10-08T15:25:44","slug":"external-experts-soc","status":"publish","type":"page","link":"https:\/\/www.issibern.ch\/teams\/blackholebinary\/external-experts-soc\/","title":{"rendered":"External experts (SOC)"},"content":{"rendered":"<ul>\n<li>P. Amaro-Seoane (University of\u00a0 Barcelona, Spain) <a href=\"mailto:pau@ice.cat\">pau@ice.cat<\/a>\n<ul style=\"list-style-type: circle\">\n<li>Relativistic astrophysics, theory<\/li>\n<\/ul>\n<\/li>\n<\/ul>\n<ul>\n<li>R. Klessen (Zentrum f\u00fcr Astronomie, Heidelberg, Germany) <a href=\"mailto:rklessen@uni-heidelberg.de?subject=\">rklessen@uni-heidelberg.de<\/a>\n<ul style=\"list-style-type: circle\">\n<li>Hydrodynamics, star formation<\/li>\n<\/ul>\n<\/li>\n<\/ul>\n<ul>\n<li>Zhanwen Han (Yunnan Astronomical Observatories, CAS, Kunming, China)\n<ul style=\"list-style-type: circle\">\n<li>Binary star evolution<\/li>\n<\/ul>\n<\/li>\n<\/ul>\n<ul>\n<li>M. Gieles (University of Surrey, U.K.)\n<ul style=\"list-style-type: circle\">\n<li>Evolution of star clusters, stellar populations<\/li>\n<\/ul>\n<\/li>\n<\/ul>\n<ul>\n<li>R. Spurzem\u00a0 (National Astronomical Observatories, CAS &amp; Kavli Institute\u00a0 of Astronomy and Astrophysics, Peking University, China) <a href=\"mailto:spurzem@nao.cas.cn\">spurzem@nao.cas.cn<\/a>\n<ul style=\"list-style-type: circle\">\n<li>Stellar dynamics, relativistic astrophysics, high-performance computing<\/li>\n<\/ul>\n<\/li>\n<\/ul>\n<ul>\n<li>G. Meynet (Observatoire de Gen\u00e8ve, Switzerland) <a href=\"mailto:georges.meynet@unige.ch\">georges.meynet@unige.ch<\/a>\n<ul style=\"list-style-type: circle\">\n<li>Stellar evolution, massive stars, mixing<\/li>\n<\/ul>\n<\/li>\n<\/ul>\n<ul>\n<li>M. Spera\u00a0 (University of Milano Bicocca, Italy)\n<ul style=\"list-style-type: circle\">\n<li>Stellar evolution, the dynamics of binary stars<\/li>\n<\/ul>\n<\/li>\n<\/ul>\n","protected":false},"excerpt":{"rendered":"<p>P. Amaro-Seoane (University of\u00a0 Barcelona, Spain) pau@ice.cat Relativistic astrophysics, theory R. Klessen (Zentrum f\u00fcr Astronomie, Heidelberg, Germany) rklessen@uni-heidelberg.de Hydrodynamics, star formation Zhanwen Han (Yunnan Astronomical Observatories, CAS, Kunming, China) Binary star evolution M. Gieles (University of Surrey, U.K.) Evolution of &hellip; <a href=\"https:\/\/www.issibern.ch\/teams\/blackholebinary\/external-experts-soc\/\">Continue reading <span class=\"meta-nav\">&rarr;<\/span><\/a><\/p>\n","protected":false},"author":2,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-17","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/www.issibern.ch\/teams\/blackholebinary\/wp-json\/wp\/v2\/pages\/17","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.issibern.ch\/teams\/blackholebinary\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/www.issibern.ch\/teams\/blackholebinary\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/www.issibern.ch\/teams\/blackholebinary\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.issibern.ch\/teams\/blackholebinary\/wp-json\/wp\/v2\/comments?post=17"}],"version-history":[{"count":0,"href":"https:\/\/www.issibern.ch\/teams\/blackholebinary\/wp-json\/wp\/v2\/pages\/17\/revisions"}],"wp:attachment":[{"href":"https:\/\/www.issibern.ch\/teams\/blackholebinary\/wp-json\/wp\/v2\/media?parent=17"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}