{"id":130,"date":"2017-02-20T16:42:23","date_gmt":"2017-02-20T14:42:23","guid":{"rendered":"http:\/\/phsites.technion.ac.il\/agn-2017\/?p=130"},"modified":"2017-06-15T09:44:28","modified_gmt":"2017-06-15T07:44:28","slug":"s-aalto-molecular-outflows-agns-starbursts","status":"publish","type":"post","link":"https:\/\/phsites.technion.ac.il\/agn-2017\/s-aalto-molecular-outflows-agns-starbursts\/","title":{"rendered":"S. Aalto – Molecular outflows in AGNs and starbursts"},"content":{"rendered":"

See Presentation<\/a><\/p>\n

    \n
  1. Can AGN-powered molecular jets appear as disk-winds similar to what we see in protostars? If so \u2013 will we then see molecular jets also in the quasar mode of accretion?<\/li>\n
  2. Is it possible that molecular jets are important processes in solving the angular momentum problem for SMBH growth \u2013 or is the jet of NGC1377 a unique phenomenon?<\/li>\n
  3. What is the fate of the gas in AGN\/starburst outflows? Can it fall back onto the galaxy again \u2013 serving as an \u201cengine\u201d for SMBH and stellar growth? If so \u2013 how is this then linked to the \u201ccold accretion\u201d hypothesis?<\/li>\n
  4. How is it possible that molecules are surviving in 1000 km\/s outflows? Are the molecules carried out from the disk, or are they formed in-situ from the hot gas?<\/li>\n
  5. What are the physical conditions of the gas in the outflow? Can the gas clumps really be self-gravitating \u2013 or are we seeing diffuse, unbound molecular gas. (A related question is if the gas can form stars in the flow). The answer to this queston is important also for the mass estimates of the cold gas, which currently has at least a factor of 10 uncertainty.<\/li>\n
  6. Are the physical conditions and ultimate fate of the gas different in AGN and starburst flows?<\/li>\n
  7. Will AGN and starburst feedback impact their host galaxies differently? Are quasars and their outflows really \u201ca waste of space\u201d? (quote from J. Binney)<\/li>\n<\/ol>\n","protected":false},"excerpt":{"rendered":"

    See Presentation Can AGN-powered molecular jets appear as disk-winds similar to what we see in protostars? If so \u2013 will we then see molecular jets also in the quasar mode of accretion? Is it possible that molecular jets are important processes in solving the angular momentum problem for SMBH growth \u2013 or is the jet …<\/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-130","1":"post","2":"type-post","3":"status-publish","4":"format-standard","6":"category-talks","7":"entry"},"yoast_head":"\nS. Aalto - Molecular outflows in AGNs and starbursts - 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-aalto-molecular-outflows-agns-starbursts\/\" \/>\n<meta property=\"og:locale\" content=\"en_US\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"S. Aalto - Molecular outflows in AGNs and starbursts - AGN Driven Winds\" \/>\n<meta property=\"og:description\" content=\"See Presentation Can AGN-powered molecular jets appear as disk-winds similar to what we see in protostars? If so \u2013 will we then see molecular jets also in the quasar mode of accretion? 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