{"id":141,"date":"2012-07-09T09:53:43","date_gmt":"2012-07-09T14:53:43","guid":{"rendered":"http:\/\/people.brandonu.ca\/gulliver\/?page_id=141"},"modified":"2012-07-09T13:34:11","modified_gmt":"2012-07-09T18:34:11","slug":"abstract-cobalt-abundances-early-type-stars","status":"publish","type":"page","link":"https:\/\/people.brandonu.ca\/gulliver\/publications\/abstract-cobalt-abundances-early-type-stars\/","title":{"rendered":"Abstract: On the Cobalt Abundances of Early Type Stars."},"content":{"rendered":"<p>Photographic region high-dispersion high signal-to-noise spectra of A and F main sequence band stars which exhibit modest rotation show Co I lines. In the hottest of these stars, we also found weak Co II lines whose abundances are consistent with those from Co I lines. As a class the Am stars have cobalt abundances which are greater than solar while the normal stars have solar values. <\/p>\n","protected":false},"excerpt":{"rendered":"<p>Photographic region high-dispersion high signal-to-noise spectra of A and F main sequence band stars which exhibit modest rotation show Co I lines. In the hottest of these stars, we also found weak Co II lines whose abundances are consistent with those from Co I lines. As a class the Am stars have cobalt abundances which [&hellip;]<\/p>\n","protected":false},"author":3,"featured_media":0,"parent":8,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-141","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/people.brandonu.ca\/gulliver\/wp-json\/wp\/v2\/pages\/141","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/people.brandonu.ca\/gulliver\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/people.brandonu.ca\/gulliver\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/people.brandonu.ca\/gulliver\/wp-json\/wp\/v2\/users\/3"}],"replies":[{"embeddable":true,"href":"https:\/\/people.brandonu.ca\/gulliver\/wp-json\/wp\/v2\/comments?post=141"}],"version-history":[{"count":3,"href":"https:\/\/people.brandonu.ca\/gulliver\/wp-json\/wp\/v2\/pages\/141\/revisions"}],"predecessor-version":[{"id":189,"href":"https:\/\/people.brandonu.ca\/gulliver\/wp-json\/wp\/v2\/pages\/141\/revisions\/189"}],"up":[{"embeddable":true,"href":"https:\/\/people.brandonu.ca\/gulliver\/wp-json\/wp\/v2\/pages\/8"}],"wp:attachment":[{"href":"https:\/\/people.brandonu.ca\/gulliver\/wp-json\/wp\/v2\/media?parent=141"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}