{"id":72,"date":"2017-02-20T12:53:12","date_gmt":"2017-02-20T10:53:12","guid":{"rendered":"http:\/\/phsites.technion.ac.il\/agn-2017\/?p=72"},"modified":"2017-06-11T07:27:34","modified_gmt":"2017-06-11T05:27:34","slug":"m-guainazzi-global-view-agn-winds-sample-studies-nearby-seyferts","status":"publish","type":"post","link":"https:\/\/phsites.technion.ac.il\/agn-2017\/m-guainazzi-global-view-agn-winds-sample-studies-nearby-seyferts\/","title":{"rendered":"M. Guainazzi &#8211; A global view of AGN winds from sample studies of nearby Seyferts"},"content":{"rendered":"<p><a class=\"uk-button \" title=\"A global view of AGN winds from sample studies of nearby Seyferts - M. Guainazzi\" href=\"http:\/\/phsites.technion.ac.il\/talks\/agn2017\/Guainazzi-M.pdf\">See Presentation<\/a><\/p>\n<p>Starting from recent X-ray studies of sizable samples of local Seyfert galaxies at moderate and high energy resolution, I will address the following questions:\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0 \u00a0<\/p>\n<ul>\n<li>Are the distributions of AGN wind physical parameters dependent on AGN luminosity or radio-loudness?<\/li>\n<li>How complete is our census of AGN winds? How many of them are we missing due to ionisation or inclination (or other) effects?<\/li>\n<li>UFOs in the post-Hitomi era: are we still seeking for an ultimate observational confirmation? Do observations of UFOs at high energy resolution support the finding at moderate (CCD) resolution?<\/li>\n<li>&#8220;Warm absorbers&#8221; vs. UFOs: two populations? Two aspects of the same underlying phenomenon?<\/li>\n<li>Are the different observational components of AGN outflows part of the same stratified flow? Are they independent components launched at different scales?<\/li>\n<li>What does the &#8220;ionisation gap&#8221; mean?<\/li>\n<li>Which observational constraints exist on the mechanism launching and accelerating the winds?<\/li>\n<li>Do AGN outflows contribute (or are responsible) for AGN obscuration?<\/li>\n<li>How uncertain are our estimates of mass\/kinetic energy\/momentum outflow rates?<\/li>\n<li>Bonus question (depending on the XRM status):<\/li>\n<li>Should XRM (X-Ray Re-flight Mission) fly, would the AGN wind observation plan originally designed for Hitomi still be adequate?<\/li>\n<\/ul>\n","protected":false},"excerpt":{"rendered":"<p>See Presentation Starting from recent X-ray studies of sizable samples of local Seyfert galaxies at moderate and high energy resolution, I will address the following questions:\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0 \u00a0 Are the distributions of AGN wind physical parameters dependent on AGN luminosity or radio-loudness? How complete is our census of AGN winds? How many of them are we &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-72","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>M. 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