{"id":90,"date":"2010-01-27T19:23:21","date_gmt":"2010-01-27T18:23:21","guid":{"rendered":"http:\/\/astronomy.lamost.org\/blog\/?page_id=90"},"modified":"2010-07-30T17:47:23","modified_gmt":"2010-07-30T15:47:23","slug":"gcm","status":"publish","type":"page","link":"http:\/\/astronomy.lamost.org\/blog\/?page_id=90","title":{"rendered":"GCM"},"content":{"rendered":"<h2><span style=\"font-weight: normal; font-size: 13px;\"><span style=\"color: #000000;\"><span style=\"color: #000000;\">Galactic\u00a0Chemical Evolution<\/span><del datetime=\"2010-01-28T18:06:59+00:00\"><\/del><\/span><\/span><\/h2>\n<div id=\"_mcePaste\" style=\"position: absolute; left: -10000px; top: 0px; width: 1px; height: 1px; overflow-x: hidden; overflow-y: hidden;\">Stars and interstellar gas in galaxies exhibit diverse chemical<\/div>\n<div id=\"_mcePaste\" style=\"position: absolute; left: -10000px; top: 0px; width: 1px; height: 1px; overflow-x: hidden; overflow-y: hidden;\">element abundance patterns that are shaped by their<\/div>\n<div id=\"_mcePaste\" style=\"position: absolute; left: -10000px; top: 0px; width: 1px; height: 1px; overflow-x: hidden; overflow-y: hidden;\">environment and formation histories. The aim of Galactic<\/div>\n<div id=\"_mcePaste\" style=\"position: absolute; left: -10000px; top: 0px; width: 1px; height: 1px; overflow-x: hidden; overflow-y: hidden;\">Chemical Evolution (GCE) is to use the observed abundances<\/div>\n<div id=\"_mcePaste\" style=\"position: absolute; left: -10000px; top: 0px; width: 1px; height: 1px; overflow-x: hidden; overflow-y: hidden;\">to unlock earlier epochs in the Universe, probe the<\/div>\n<div id=\"_mcePaste\" style=\"position: absolute; left: -10000px; top: 0px; width: 1px; height: 1px; overflow-x: hidden; overflow-y: hidden;\">mechanisms of galaxy formation, and gain insight into the<\/div>\n<div id=\"_mcePaste\" style=\"position: absolute; left: -10000px; top: 0px; width: 1px; height: 1px; overflow-x: hidden; overflow-y: hidden;\">evolution of stellar systems.<\/div>\n<div style=\"text-align: left;\"><em>Stars and interstellar gas in galaxies exhibit diverse chemical\u00a0element abundance patterns that are shaped by their<\/em><\/div>\n<div style=\"text-align: left;\"><em>environment and formation histories. The aim of Galactic\u00a0Chemical Evolution (GCE) is to use the observed abundances<\/em><\/div>\n<div style=\"text-align: left;\"><em>to unlock earlier epochs in the Universe, probe the\u00a0mechanisms of galaxy formation, and gain insight into the\u00a0evolution of stellar systems. \uff08Gibson \uff5e2003\uff09<\/em><\/div>\n<h2 style=\"text-align: justify;\">GCM Ingredients<\/h2>\n<p>IMF<\/p>\n<p>SFR<\/p>\n<p>Stellar Yield<\/p>\n<p>Stellar life time<\/p>\n<p>Energy\u00a0component<\/p>\n<h2>Phenomenology<\/h2>\n<p>LBG<\/p>\n<p>QSO<\/p>\n<p>GRB<\/p>\n<h2>Morphology<\/h2>\n<p>Elliptical<\/p>\n<h2>My work<\/h2>\n<p><span style=\"font-family: 'Lucida Grande', helvetica, arial, verdana, sans-serif; line-height: normal; font-size: 14px;\"><a href=\"http:\/\/arxiv.org\/abs\/1007.4435\" target=\"_blank\">The nature of Long-GRB host galaxies from chemical abundances<\/a><\/p>\n<p><\/span><\/p>\n","protected":false},"excerpt":{"rendered":"<p>Galactic\u00a0Chemical Evolution Stars and interstellar gas &#8230;<\/p>\n","protected":false},"author":2,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"open","ping_status":"open","template":"","meta":{"footnotes":""},"class_list":["post-90","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"http:\/\/astronomy.lamost.org\/blog\/index.php?rest_route=\/wp\/v2\/pages\/90","targetHints":{"allow":["GET"]}}],"collection":[{"href":"http:\/\/astronomy.lamost.org\/blog\/index.php?rest_route=\/wp\/v2\/pages"}],"about":[{"href":"http:\/\/astronomy.lamost.org\/blog\/index.php?rest_route=\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"http:\/\/astronomy.lamost.org\/blog\/index.php?rest_route=\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"http:\/\/astronomy.lamost.org\/blog\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=90"}],"version-history":[{"count":13,"href":"http:\/\/astronomy.lamost.org\/blog\/index.php?rest_route=\/wp\/v2\/pages\/90\/revisions"}],"predecessor-version":[{"id":92,"href":"http:\/\/astronomy.lamost.org\/blog\/index.php?rest_route=\/wp\/v2\/pages\/90\/revisions\/92"}],"wp:attachment":[{"href":"http:\/\/astronomy.lamost.org\/blog\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=90"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}