{"id":79,"date":"2010-01-27T19:02:04","date_gmt":"2010-01-27T18:02:04","guid":{"rendered":"http:\/\/astronomy.lamost.org\/blog\/?page_id=79"},"modified":"2011-05-11T17:35:18","modified_gmt":"2011-05-11T15:35:18","slug":"dust","status":"publish","type":"page","link":"http:\/\/astronomy.lamost.org\/blog\/?page_id=79","title":{"rendered":"Dust"},"content":{"rendered":"<h2><span style=\"color: #000000;\">Conference<\/span><\/h2>\n<p><a href=\"http:\/\/www.aspbooks.org\/a\/volumes\/table_of_contents\/?book_id=16\">Astrophysics of Dust<\/a><\/p>\n<p><a style=\"font-family: arial, sans-serif; color: #551a8b;\" onmousedown=\"return clk(this.href,'','','res','4','&amp;sig2=2bZgUfqmqjfA2KFtBncxOw','0CCEQFjAD')\" href=\"http:\/\/www.iiap.res.in\/dust\">Physics and\u00a0<em>Astrophysics of Dust<\/em> II<\/a><\/p>\n<p><span style=\"font-family: 'Lucida Grande', helvetica, arial, verdana, sans-serif; line-height: normal; -webkit-border-horizontal-spacing: 2px; -webkit-border-vertical-spacing: 2px;\"><a href=\"http:\/\/www.mpia-hd.mpg.de\/DNF08\/\">Cosmic Dust &#8211; Near and Far<\/a><\/span><\/p>\n<h2><span style=\"color: #000000;\">Book<\/span><\/h2>\n<h2>Dust sources<\/h2>\n<p>evolved stellar<\/p>\n<p>SN<\/p>\n<p>QSO<\/p>\n<h2>Dust evolution in ISM<\/h2>\n<p>dust destruction<\/p>\n<p>dust growth<\/p>\n<h2>Interstellar Dust Models<\/h2>\n<p>At this point, it is not possible to \u201cinvert\u201d the observations to \u201cderive\u201d the\u00a0nature of interstellar dust \u2013 neither theory nor observations are good enough.\u00a0The only feasible approach is to propose a dust model, calculate its properties,\u00a0and compare it to observations. If the model disagrees with the observations, it\u00a0is rejected. (<span style=\"font-family: arial; line-height: normal; font-size: 14px; color: #000044; -webkit-border-horizontal-spacing: 3px; -webkit-border-vertical-spacing: 3px;\">Draine, B.T.2004)<\/span><\/p>\n<p>dust\u00a0composition<\/p>\n<p><span style=\"line-height: normal; font-size: xx-small;\">Size distribution<\/span><\/p>\n<p><span style=\"line-height: normal; font-size: xx-small;\"><br \/>\n<\/span><\/p>\n<p><span style=\"line-height: normal; font-size: xx-small;\"><span style=\"font-family: Simsun; font-size: small;\"> <\/span><\/span><\/p>\n<h2><a href=\"http:\/\/webast.ast.obs-mip.fr\/hyperz\/hyperz_manual1\/node10.html#figred\">Reddening<\/a><\/h2>\n<h2><\/h2>\n<h2>\u79d1\u666e<\/h2>\n<h2><a href=\"http:\/\/www.astro.cardiff.ac.uk\/pub\/Steve.Eales\/Sky-and-Telescope.pdf\">Smoking Supernovae<\/a><\/h2>\n<p><span style=\"line-height: normal; font-size: x-small;\"> <\/span><\/p>\n<div id=\"_mcePaste\" style=\"position: absolute; left: -10000px; top: 123px; width: 1px; height: 1px; overflow: hidden;\">At this point, it is not possible to \u201cinvert\u201d the observations to \u201cderive\u201d the<\/div>\n<div id=\"_mcePaste\" style=\"position: absolute; left: -10000px; top: 123px; width: 1px; height: 1px; overflow: hidden;\">nature of interstellar dust \u2013 neither theory nor observations are good enough.<\/div>\n<div id=\"_mcePaste\" style=\"position: absolute; left: -10000px; top: 123px; width: 1px; height: 1px; overflow: hidden;\">The only feasible approach is to propose a dust model, calculate its properties,<\/div>\n<div id=\"_mcePaste\" style=\"position: absolute; left: -10000px; top: 123px; width: 1px; height: 1px; overflow: hidden;\">and compare it to observations. If the model disagrees with the observations, it<\/div>\n<div id=\"_mcePaste\" style=\"position: absolute; left: -10000px; top: 123px; width: 1px; height: 1px; overflow: hidden;\">is rejectedAt this point, it is not possible to \u201cinvert\u201d the observations to \u201cderive\u201d the<\/div>\n<div id=\"_mcePaste\" style=\"position: absolute; left: -10000px; top: 123px; width: 1px; height: 1px; overflow: hidden;\">nature of interstellar dust \u2013 neither theory nor observations are good enough.<\/div>\n<div id=\"_mcePaste\" style=\"position: absolute; left: -10000px; top: 123px; width: 1px; height: 1px; overflow: hidden;\">The only feasible approach is to propose a dust model, calculate its properties,<\/div>\n<div id=\"_mcePaste\" style=\"position: absolute; left: -10000px; top: 123px; width: 1px; height: 1px; overflow: hidden;\">and compare it to observations. If the model disagrees with the observations, it<\/div>\n<div id=\"_mcePaste\" style=\"position: absolute; left: -10000px; top: 123px; width: 1px; height: 1px; overflow: hidden;\">is rejected.<\/div>\n","protected":false},"excerpt":{"rendered":"<p>Conference Astrophysics of Dust Physics and\u00a0Astrophysic&#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-79","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"http:\/\/astronomy.lamost.org\/blog\/index.php?rest_route=\/wp\/v2\/pages\/79","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=79"}],"version-history":[{"count":17,"href":"http:\/\/astronomy.lamost.org\/blog\/index.php?rest_route=\/wp\/v2\/pages\/79\/revisions"}],"predecessor-version":[{"id":332,"href":"http:\/\/astronomy.lamost.org\/blog\/index.php?rest_route=\/wp\/v2\/pages\/79\/revisions\/332"}],"wp:attachment":[{"href":"http:\/\/astronomy.lamost.org\/blog\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=79"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}