{"id":132,"date":"2017-02-20T16:43:23","date_gmt":"2017-02-20T14:43:23","guid":{"rendered":"http:\/\/phsites.technion.ac.il\/agn-2017\/?p=132"},"modified":"2017-06-11T07:50:35","modified_gmt":"2017-06-11T05:50:35","slug":"r-maiolino-negative-positive-agn-feedback","status":"publish","type":"post","link":"https:\/\/phsites.technion.ac.il\/agn-2017\/r-maiolino-negative-positive-agn-feedback\/","title":{"rendered":"R. Maiolino &#8211; Negative and positive AGN feedback"},"content":{"rendered":"<p><a class=\"uk-button \" title=\"R. Maiolino - Negative and positive AGN feedback\" href=\"http:\/\/phsites.technion.ac.il\/talks\/agn2017\/Maiolino_R.pdf\">See Presentation<\/a><\/p>\n<p>I will present some observational results illustrating the properties of AGN-driven outflows and their effect on star formation in their host galaxies. In particular I will present multi-band observations<\/p>\n<p>tracing both the molecular and ionized phase of the ISM, both in local and distant galaxies, illustrating that AGNs can drive extremely powerful and energetic outflows, which can expel a large fraction<\/p>\n<p>of the gas in their host galaxies, hence suppressing star formation (negative feedback). However, I will also show evidence that in some cases AGN-driven outflows can actually trigger star formation, both in their host galaxy discs and even in the outflow itself. This is a new mode of star formation, which can contribute significantly to galaxy evolution. I will conclude by presenting the exciting prospects of further investigating these effects in the near future.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>See Presentation I will present some observational results illustrating the properties of AGN-driven outflows and their effect on star formation in their host galaxies. In particular I will present multi-band observations tracing both the molecular and ionized phase of the ISM, both in local and distant galaxies, illustrating that AGNs can drive extremely powerful and &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-132","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>R. Maiolino - Negative and positive AGN feedback - 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\/r-maiolino-negative-positive-agn-feedback\/\" \/>\n<meta property=\"og:locale\" content=\"en_US\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"R. Maiolino - Negative and positive AGN feedback - AGN Driven Winds\" \/>\n<meta property=\"og:description\" content=\"See Presentation I will present some observational results illustrating the properties of AGN-driven outflows and their effect on star formation in their host galaxies. In particular I will present multi-band observations tracing both the molecular and ionized phase of the ISM, both in local and distant galaxies, illustrating that AGNs can drive extremely powerful and &hellip;\" \/>\n<meta property=\"og:url\" content=\"https:\/\/phsites.technion.ac.il\/agn-2017\/r-maiolino-negative-positive-agn-feedback\/\" \/>\n<meta property=\"og:site_name\" content=\"AGN Driven Winds\" \/>\n<meta property=\"article:published_time\" content=\"2017-02-20T14:43:23+00:00\" \/>\n<meta property=\"article:modified_time\" content=\"2017-06-11T05:50:35+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\t<meta name=\"twitter:label2\" content=\"Est. reading time\" \/>\n\t<meta name=\"twitter:data2\" content=\"1 minute\" \/>\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\\\/r-maiolino-negative-positive-agn-feedback\\\/#article\",\"isPartOf\":{\"@id\":\"https:\\\/\\\/phsites.technion.ac.il\\\/agn-2017\\\/r-maiolino-negative-positive-agn-feedback\\\/\"},\"author\":{\"name\":\"Adi\",\"@id\":\"https:\\\/\\\/phsites.technion.ac.il\\\/agn-2017\\\/#\\\/schema\\\/person\\\/65231d9f0ecb94f8411926c66a3791ff\"},\"headline\":\"R. 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