{"id":2,"date":"2021-01-25T16:31:45","date_gmt":"2021-01-25T15:31:45","guid":{"rendered":"https:\/\/www.oa-roma.inaf.it\/arca\/?page_id=2"},"modified":"2021-04-14T14:37:28","modified_gmt":"2021-04-14T12:37:28","slug":"pagina-di-esempio","status":"publish","type":"page","link":"https:\/\/www.oa-roma.inaf.it\/arca\/","title":{"rendered":"Welcome!"},"content":{"rendered":"\n<p>This website is the repository of the stellar evolution models computed with the code ATON (<a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/1991ApJ...370..295C\/\/abstract\">Canuto&amp; Mazzitelli, 1991<\/a>; <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/1998A&amp;A...334..953V\/abstract\">Ventura et al. 1998<\/a>). It contains physical, chemical and dust evolutionary sequences, gas and dust yields for the metallicities listed below.<\/p>\n\n\n\n<ul class=\"wp-block-list\"><li>[Fe\/H]=-3 (Z=3 *10<sup>-5<\/sup>)  [<a href=\"https:\/\/www.oa-roma.inaf.it\/arca\/fe-h-3\/\">link to the page<\/a>]<\/li><li>[Fe\/H]=-5 (Z=3*10<sup>-7<\/sup>)   [<a href=\"https:\/\/www.oa-roma.inaf.it\/arca\/fe-h-5\/\">link to the page<\/a>]<\/li><\/ul>\n\n\n\n<p><\/p>\n","protected":false},"excerpt":{"rendered":"<p>This website is the repository of the stellar evolution models computed with the code ATON (Canuto&amp; Mazzitelli, 1991; Ventura et al. 1998). It contains physical, chemical and dust evolutionary sequences, gas and dust yields for the metallicities listed below. [Fe\/H]=-3 (Z=3 *10-5) [link to the page] [Fe\/H]=-5 (Z=3*10-7) [link to the page]<\/p>\n","protected":false},"author":89,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"open","template":"","meta":{"_acf_changed":false,"footnotes":""},"class_list":["post-2","page","type-page","status-publish","hentry"],"acf":[],"_links":{"self":[{"href":"https:\/\/www.oa-roma.inaf.it\/arca\/wp-json\/wp\/v2\/pages\/2","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.oa-roma.inaf.it\/arca\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/www.oa-roma.inaf.it\/arca\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/www.oa-roma.inaf.it\/arca\/wp-json\/wp\/v2\/users\/89"}],"replies":[{"embeddable":true,"href":"https:\/\/www.oa-roma.inaf.it\/arca\/wp-json\/wp\/v2\/comments?post=2"}],"version-history":[{"count":18,"href":"https:\/\/www.oa-roma.inaf.it\/arca\/wp-json\/wp\/v2\/pages\/2\/revisions"}],"predecessor-version":[{"id":61,"href":"https:\/\/www.oa-roma.inaf.it\/arca\/wp-json\/wp\/v2\/pages\/2\/revisions\/61"}],"wp:attachment":[{"href":"https:\/\/www.oa-roma.inaf.it\/arca\/wp-json\/wp\/v2\/media?parent=2"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}