{"id":110,"date":"2017-02-20T16:21:29","date_gmt":"2017-02-20T14:21:29","guid":{"rendered":"http:\/\/phsites.technion.ac.il\/agn-2017\/?p=110"},"modified":"2017-06-11T12:48:43","modified_gmt":"2017-06-11T10:48:43","slug":"s-davis-simulations-accretion-flows-grey-opacities","status":"publish","type":"post","link":"https:\/\/phsites.technion.ac.il\/agn-2017\/s-davis-simulations-accretion-flows-grey-opacities\/","title":{"rendered":"S. Davis &#8211; Simulations of accretion flows with grey opacities"},"content":{"rendered":"<p><a class=\"uk-button \" title=\"S. Davis - Simulations of accretion flows with grey opacities\" href=\"http:\/\/phsites.technion.ac.il\/talks\/agn2017\/Davis-S.pdf\">See Presentation<\/a><\/p>\n<p>What role does UV opacity play in the structure and evolution of accretion disks? \u00a0What can simulations tell us about how winds are launched by radiation and, in particular, how that launching feeds back on the disk structure? \u00a0Given the limits of numerical simulations, how can we best design the simulations that address these issues? \u00a0Do the outflows being launched at relatively small radii in accretion disk simulations connect with either the broad absorption line quasars or ultrafast outflows?<\/p>\n","protected":false},"excerpt":{"rendered":"<p>See Presentation What role does UV opacity play in the structure and evolution of accretion disks? \u00a0What can simulations tell us about how winds are launched by radiation and, in particular, how that launching feeds back on the disk structure? \u00a0Given the limits of numerical simulations, how can we best design the simulations that address &hellip;<\/p>\n","protected":false},"author":2,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"_genesis_hide_title":false,"_genesis_hide_breadcrumbs":false,"_genesis_hide_singular_image":false,"_genesis_hide_footer_widgets":false,"_genesis_custom_body_class":"","_genesis_custom_post_class":"","_genesis_layout":"","footnotes":""},"categories":[3],"tags":[],"class_list":{"0":"post-110","1":"post","2":"type-post","3":"status-publish","4":"format-standard","6":"category-talks","7":"entry"},"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v27.6 - https:\/\/yoast.com\/product\/yoast-seo-wordpress\/ -->\n<title>S. Davis - Simulations of accretion flows with grey opacities - AGN Driven Winds<\/title>\n<meta name=\"robots\" content=\"index, follow, max-snippet:-1, max-image-preview:large, max-video-preview:-1\" \/>\n<link rel=\"canonical\" href=\"https:\/\/phsites.technion.ac.il\/agn-2017\/s-davis-simulations-accretion-flows-grey-opacities\/\" \/>\n<meta property=\"og:locale\" content=\"en_US\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"S. Davis - Simulations of accretion flows with grey opacities - AGN Driven Winds\" \/>\n<meta property=\"og:description\" content=\"See Presentation What role does UV opacity play in the structure and evolution of accretion disks? \u00a0What can simulations tell us about how winds are launched by radiation and, in particular, how that launching feeds back on the disk structure? \u00a0Given the limits of numerical simulations, how can we best design the simulations that address &hellip;\" \/>\n<meta property=\"og:url\" content=\"https:\/\/phsites.technion.ac.il\/agn-2017\/s-davis-simulations-accretion-flows-grey-opacities\/\" \/>\n<meta property=\"og:site_name\" content=\"AGN Driven Winds\" \/>\n<meta property=\"article:published_time\" content=\"2017-02-20T14:21:29+00:00\" \/>\n<meta property=\"article:modified_time\" content=\"2017-06-11T10:48:43+00:00\" \/>\n<meta name=\"author\" content=\"Adi\" \/>\n<meta name=\"twitter:card\" content=\"summary_large_image\" \/>\n<meta name=\"twitter:label1\" content=\"Written by\" \/>\n\t<meta name=\"twitter:data1\" content=\"Adi\" \/>\n<script type=\"application\/ld+json\" class=\"yoast-schema-graph\">{\"@context\":\"https:\\\/\\\/schema.org\",\"@graph\":[{\"@type\":\"Article\",\"@id\":\"https:\\\/\\\/phsites.technion.ac.il\\\/agn-2017\\\/s-davis-simulations-accretion-flows-grey-opacities\\\/#article\",\"isPartOf\":{\"@id\":\"https:\\\/\\\/phsites.technion.ac.il\\\/agn-2017\\\/s-davis-simulations-accretion-flows-grey-opacities\\\/\"},\"author\":{\"name\":\"Adi\",\"@id\":\"https:\\\/\\\/phsites.technion.ac.il\\\/agn-2017\\\/#\\\/schema\\\/person\\\/65231d9f0ecb94f8411926c66a3791ff\"},\"headline\":\"S. 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