% $ biblatex auxiliary file $
% $ biblatex bbl format version 2.8 $
% Do not modify the above lines!
%
% This is an auxiliary file used by the 'biblatex' package.
% This file may safely be deleted. It will be recreated by
% biber as required.
%
\begingroup
\makeatletter
\@ifundefined{ver@biblatex.sty}
  {\@latex@error
     {Missing 'biblatex' package}
     {The bibliography requires the 'biblatex' package.}
      \aftergroup\endinput}
  {}
\endgroup


\refsection{0}
  \sortlist[entry]{nty/global/}
    \entry{2016ASSL..418..317B}{article}{}
      \name{author}{2}{}{%
        {{hash=1aeeb5895153e5067de0ada27080d279}{%
           family={{Brooks}},
           familyi={B\bibinitperiod},
           given={A.},
           giveni={A\bibinitperiod}}}%
        {{hash=18c425f06f5f16e04da4e875cf33cdd2}{%
           family={{Christensen}},
           familyi={C\bibinitperiod},
           given={C.},
           giveni={C\bibinitperiod}}}%
      }
      \strng{namehash}{fdd52e36dc9e22ff2de8d164876037cd}
      \strng{fullhash}{fdd52e36dc9e22ff2de8d164876037cd}
      \strng{authornamehash}{fdd52e36dc9e22ff2de8d164876037cd}
      \strng{authorfullhash}{fdd52e36dc9e22ff2de8d164876037cd}
      \field{sortinit}{B}
      \field{sortinithash}{5f6fa000f686ee5b41be67ba6ff7962d}
      \field{labelnamesource}{author}
      \field{labeltitlesource}{title}
      \field{eprinttype}{arXiv}
      \field{journaltitle}{Galactic Bulges}
      \field{title}{{Bulge Formation via Mergers in Cosmological Simulations}}
      \field{volume}{418}
      \field{year}{2016}
      \field{pages}{317}
      \range{pages}{1}
      \verb{doi}
      \verb 10.1007/978-3-319-19378-6_12
      \endverb
      \verb{eprint}
      \verb 1511.04095
      \endverb
      \keyw{Physics}
    \endentry
    \entry{2016IAUS..319...17G}{inproceedings}{}
      \name{author}{1}{}{%
        {{hash=565f911e6e07bbd8826f2a2d08d6a856}{%
           family={{Gaspari}},
           familyi={G\bibinitperiod},
           given={M.},
           giveni={M\bibinitperiod}}}%
      }
      \name{editor}{1}{}{%
        {{hash=b53a42d44643a9d2879a568ba135dda8}{%
           family={{Kaviraj}},
           familyi={K\bibinitperiod},
           given={S.},
           giveni={S\bibinitperiod}}}%
      }
      \strng{namehash}{565f911e6e07bbd8826f2a2d08d6a856}
      \strng{fullhash}{565f911e6e07bbd8826f2a2d08d6a856}
      \strng{authornamehash}{565f911e6e07bbd8826f2a2d08d6a856}
      \strng{authorfullhash}{565f911e6e07bbd8826f2a2d08d6a856}
      \strng{editornamehash}{b53a42d44643a9d2879a568ba135dda8}
      \strng{editorfullhash}{b53a42d44643a9d2879a568ba135dda8}
      \field{sortinit}{G}
      \field{sortinithash}{618d986594b7198ba52cf8b00d348f3f}
      \field{labelnamesource}{author}
      \field{labeltitlesource}{title}
      \field{booktitle}{Galaxies at High Redshift and Their Evolution Over Cosmic Time}
      \field{eprinttype}{arXiv}
      \field{series}{IAU Symposium}
      \field{title}{{The self-regulated AGN feedback loop: the role of chaotic cold accretion}}
      \field{volume}{319}
      \field{year}{2016}
      \field{pages}{17\bibrangedash 20}
      \range{pages}{4}
      \verb{doi}
      \verb 10.1017/S1743921315010455
      \endverb
      \verb{eprint}
      \verb 1511.02871
      \endverb
      \keyw{Black hole physics,hydrodynamics,turbulence,cooling flows,galaxies: active}
    \endentry
    \entry{2017arXiv170306889H}{article}{}
      \name{author}{1}{}{%
        {{hash=7fe1a99bf1c9bd0b1bf9b081346873f6}{%
           family={{Harrison}},
           familyi={H\bibinitperiod},
           given={C.\bibnamedelimi M.},
           giveni={C\bibinitperiod\bibinitdelim M\bibinitperiod}}}%
      }
      \strng{namehash}{7fe1a99bf1c9bd0b1bf9b081346873f6}
      \strng{fullhash}{7fe1a99bf1c9bd0b1bf9b081346873f6}
      \strng{authornamehash}{7fe1a99bf1c9bd0b1bf9b081346873f6}
      \strng{authorfullhash}{7fe1a99bf1c9bd0b1bf9b081346873f6}
      \field{sortinit}{H}
      \field{sortinithash}{2f664b453ec75da1fe3804ca92633405}
      \field{labelnamesource}{author}
      \field{labeltitlesource}{title}
      \field{eprinttype}{arXiv}
      \field{journaltitle}{ArXiv e-prints}
      \field{month}{3}
      \field{title}{{Impact of supermassive black hole growth on star formation}}
      \field{year}{2017}
      \verb{eprint}
      \verb 1703.06889
      \endverb
      \keyw{Astrophysics - Astrophysics of Galaxies,Astrophysics - Cosmology and Nongalactic Astrophysics}
    \endentry
    \entry{2006ApJS..163....1H}{article}{}
      \name{author}{6}{}{%
        {{hash=e02c890164993ca28e276741a834febb}{%
           family={{Hopkins}},
           familyi={H\bibinitperiod},
           given={P.\bibnamedelimi F.},
           giveni={P\bibinitperiod\bibinitdelim F\bibinitperiod}}}%
        {{hash=49883980adbb993066f572123bf76ac1}{%
           family={{Hernquist}},
           familyi={H\bibinitperiod},
           given={L.},
           giveni={L\bibinitperiod}}}%
        {{hash=f87f6081365ab98d5a2e92d78b8048c6}{%
           family={{Cox}},
           familyi={C\bibinitperiod},
           given={T.\bibnamedelimi J.},
           giveni={T\bibinitperiod\bibinitdelim J\bibinitperiod}}}%
        {{hash=b003d5a5ab03efd2e23399948d4e4011}{%
           family={{Di Matteo}},
           familyi={D\bibinitperiod},
           given={T.},
           giveni={T\bibinitperiod}}}%
        {{hash=065f7190e1ba0526a8ed9fbbb07553d4}{%
           family={{Robertson}},
           familyi={R\bibinitperiod},
           given={B.},
           giveni={B\bibinitperiod}}}%
        {{hash=0ef85848ecf64b63065e7d36351e48f4}{%
           family={{Springel}},
           familyi={S\bibinitperiod},
           given={V.},
           giveni={V\bibinitperiod}}}%
      }
      \strng{namehash}{708948393de4aae7a796de4003e433e8}
      \strng{fullhash}{fb266c33775a4056605b1dc41483ad13}
      \strng{authornamehash}{708948393de4aae7a796de4003e433e8}
      \strng{authorfullhash}{fb266c33775a4056605b1dc41483ad13}
      \field{sortinit}{H}
      \field{sortinithash}{2f664b453ec75da1fe3804ca92633405}
      \field{labelnamesource}{author}
      \field{labeltitlesource}{title}
      \field{journaltitle}{\apjs}
      \field{month}{3}
      \field{title}{{A Unified, Merger-driven Model of the Origin of Starbursts, Quasars, the Cosmic X-Ray Background, Supermassive Black Holes, and Galaxy Spheroids}}
      \field{volume}{163}
      \field{year}{2006}
      \field{pages}{1\bibrangedash 49}
      \range{pages}{49}
      \verb{doi}
      \verb 10.1086/499298
      \endverb
      \verb{eprint}
      \verb astro-ph/0506398
      \endverb
      \keyw{Cosmology: Theory,Galaxies: Active,Galaxies: Evolution,Galaxies: Nuclei,Galaxies: Quasars: General}
    \endentry
    \entry{koristafeedback}{unpublished}{}
      \name{author}{1}{}{%
        {{hash=e6a52632505cc4f496ebb0c6b633b1c2}{%
           family={Korista},
           familyi={K\bibinitperiod},
           given={Kirk},
           giveni={K\bibinitperiod}}}%
      }
      \list{organization}{1}{%
        {Western Michigan University}%
      }
      \strng{namehash}{e6a52632505cc4f496ebb0c6b633b1c2}
      \strng{fullhash}{e6a52632505cc4f496ebb0c6b633b1c2}
      \strng{authornamehash}{e6a52632505cc4f496ebb0c6b633b1c2}
      \strng{authorfullhash}{e6a52632505cc4f496ebb0c6b633b1c2}
      \field{sortinit}{K}
      \field{sortinithash}{4c244ceae61406cdc0cc2ce1cb1ff703}
      \field{labelnamesource}{author}
      \field{labeltitlesource}{title}
      \field{month}{3}
      \field{note}{Conference presentation}
      \field{title}{Quasars and the Birth \& Evolution of Galaxies}
      \field{year}{2016}
    \endentry
    \entry{maoz2007astrophysics}{book}{}
      \name{author}{1}{}{%
        {{hash=bc495d0ee373d4cf9cffb00ee60e345d}{%
           family={Maoz},
           familyi={M\bibinitperiod},
           given={D.},
           giveni={D\bibinitperiod}}}%
      }
      \list{publisher}{1}{%
        {Princeton University Press}%
      }
      \strng{namehash}{bc495d0ee373d4cf9cffb00ee60e345d}
      \strng{fullhash}{bc495d0ee373d4cf9cffb00ee60e345d}
      \strng{authornamehash}{bc495d0ee373d4cf9cffb00ee60e345d}
      \strng{authorfullhash}{bc495d0ee373d4cf9cffb00ee60e345d}
      \field{sortinit}{M}
      \field{sortinithash}{c26a05ef03e4429073ed5c825140fac3}
      \field{labelnamesource}{author}
      \field{labeltitlesource}{title}
      \field{isbn}{9780691125848}
      \field{series}{In a Nutshell}
      \field{title}{Astrophysics in a Nutshell}
      \field{year}{2007}
      \verb{url}
      \verb https://books.google.com/books?id=r88PAQAAMAAJ
      \endverb
    \endentry
    \entry{2006ApJ...645.1092Q}{article}{}
      \name{author}{6}{}{%
        {{hash=d54b4d6c9af9184f45eedf6a2f5c6c29}{%
           family={{Quillen}},
           familyi={Q\bibinitperiod},
           given={A.\bibnamedelimi C.},
           giveni={A\bibinitperiod\bibinitdelim C\bibinitperiod}}}%
        {{hash=2e6a12f721a0527bc75b06a13818de16}{%
           family={{Brookes}},
           familyi={B\bibinitperiod},
           given={M.\bibnamedelimi H.},
           giveni={M\bibinitperiod\bibinitdelim H\bibinitperiod}}}%
        {{hash=9d67b76b8926ca646a54f924bc45208b}{%
           family={{Keene}},
           familyi={K\bibinitperiod},
           given={J.},
           giveni={J\bibinitperiod}}}%
        {{hash=0a1eb291c8eb8f13ccfaa313d2d2eefc}{%
           family={{Stern}},
           familyi={S\bibinitperiod},
           given={D.},
           giveni={D\bibinitperiod}}}%
        {{hash=11585683efabe391ec79f4e7fc09b8f8}{%
           family={{Lawrence}},
           familyi={L\bibinitperiod},
           given={C.\bibnamedelimi R.},
           giveni={C\bibinitperiod\bibinitdelim R\bibinitperiod}}}%
        {{hash=a33d8ff5959c4d5dea445d410c1122e2}{%
           family={{Werner}},
           familyi={W\bibinitperiod},
           given={M.\bibnamedelimi W.},
           giveni={M\bibinitperiod\bibinitdelim W\bibinitperiod}}}%
      }
      \strng{namehash}{a5030a4937b5486b002f314f32716bbf}
      \strng{fullhash}{2e85d74be2d7b73345a2f9a0ae282955}
      \strng{authornamehash}{a5030a4937b5486b002f314f32716bbf}
      \strng{authorfullhash}{2e85d74be2d7b73345a2f9a0ae282955}
      \field{sortinit}{Q}
      \field{sortinithash}{605f5784956f0b01c606746ceb816bf5}
      \field{labelnamesource}{author}
      \field{labeltitlesource}{title}
      \field{journaltitle}{\apj}
      \field{month}{7}
      \field{title}{{Spitzer Observations of the Dusty Warped Disk of Centaurus A}}
      \field{volume}{645}
      \field{year}{2006}
      \field{pages}{1092\bibrangedash 1101}
      \range{pages}{10}
      \verb{doi}
      \verb 10.1086/504418
      \endverb
      \verb{eprint}
      \verb astro-ph/0601135
      \endverb
      \keyw{Galaxies: Individual: NGC Number: NGC 5128,Galaxies: ISM,Galaxies: Peculiar,Galaxies: Structure}
    \endentry
    \entry{2006MNRAS.366..397S}{article}{}
      \name{author}{2}{}{%
        {{hash=13cd358daf954b37758055c05a0034cf}{%
           family={{Sijacki}},
           familyi={S\bibinitperiod},
           given={D.},
           giveni={D\bibinitperiod}}}%
        {{hash=0ef85848ecf64b63065e7d36351e48f4}{%
           family={{Springel}},
           familyi={S\bibinitperiod},
           given={V.},
           giveni={V\bibinitperiod}}}%
      }
      \strng{namehash}{fbed0411cd9a6e3d7c642ea070d5f409}
      \strng{fullhash}{fbed0411cd9a6e3d7c642ea070d5f409}
      \strng{authornamehash}{fbed0411cd9a6e3d7c642ea070d5f409}
      \strng{authorfullhash}{fbed0411cd9a6e3d7c642ea070d5f409}
      \field{sortinit}{S}
      \field{sortinithash}{3c1547c63380458f8ca90e40ed14b83e}
      \field{labelnamesource}{author}
      \field{labeltitlesource}{title}
      \field{journaltitle}{\mnras}
      \field{month}{2}
      \field{title}{{Hydrodynamical simulations of cluster formation with central AGN heating}}
      \field{volume}{366}
      \field{year}{2006}
      \field{pages}{397\bibrangedash 416}
      \range{pages}{20}
      \verb{doi}
      \verb 10.1111/j.1365-2966.2005.09860.x
      \endverb
      \verb{eprint}
      \verb astro-ph/0509506
      \endverb
      \keyw{methods: numerical,galaxies: clusters: general,cooling flows,cosmology: theory}
    \endentry
    \entry{2005ApJ...620L..79S}{article}{}
      \name{author}{3}{}{%
        {{hash=0ef85848ecf64b63065e7d36351e48f4}{%
           family={{Springel}},
           familyi={S\bibinitperiod},
           given={V.},
           giveni={V\bibinitperiod}}}%
        {{hash=b003d5a5ab03efd2e23399948d4e4011}{%
           family={{Di Matteo}},
           familyi={D\bibinitperiod},
           given={T.},
           giveni={T\bibinitperiod}}}%
        {{hash=49883980adbb993066f572123bf76ac1}{%
           family={{Hernquist}},
           familyi={H\bibinitperiod},
           given={L.},
           giveni={L\bibinitperiod}}}%
      }
      \strng{namehash}{21795803f309dd45c263dfc3828044fc}
      \strng{fullhash}{21795803f309dd45c263dfc3828044fc}
      \strng{authornamehash}{21795803f309dd45c263dfc3828044fc}
      \strng{authorfullhash}{21795803f309dd45c263dfc3828044fc}
      \field{sortinit}{S}
      \field{sortinithash}{3c1547c63380458f8ca90e40ed14b83e}
      \field{labelnamesource}{author}
      \field{labeltitlesource}{title}
      \field{journaltitle}{\apjl}
      \field{month}{2}
      \field{title}{{Black Holes in Galaxy Mergers: The Formation of Red Elliptical Galaxies}}
      \field{volume}{620}
      \field{year}{2005}
      \field{pages}{L79\bibrangedash L82}
      \range{pages}{-1}
      \verb{doi}
      \verb 10.1086/428772
      \endverb
      \verb{eprint}
      \verb astro-ph/0409436
      \endverb
      \keyw{Cosmology: Theory,Galaxies: Formation,Methods: Numerical}
    \endentry
    \entry{2005MNRAS.361..776S}{article}{}
      \name{author}{3}{}{%
        {{hash=0ef85848ecf64b63065e7d36351e48f4}{%
           family={{Springel}},
           familyi={S\bibinitperiod},
           given={V.},
           giveni={V\bibinitperiod}}}%
        {{hash=b003d5a5ab03efd2e23399948d4e4011}{%
           family={{Di Matteo}},
           familyi={D\bibinitperiod},
           given={T.},
           giveni={T\bibinitperiod}}}%
        {{hash=49883980adbb993066f572123bf76ac1}{%
           family={{Hernquist}},
           familyi={H\bibinitperiod},
           given={L.},
           giveni={L\bibinitperiod}}}%
      }
      \strng{namehash}{21795803f309dd45c263dfc3828044fc}
      \strng{fullhash}{21795803f309dd45c263dfc3828044fc}
      \strng{authornamehash}{21795803f309dd45c263dfc3828044fc}
      \strng{authorfullhash}{21795803f309dd45c263dfc3828044fc}
      \field{sortinit}{S}
      \field{sortinithash}{3c1547c63380458f8ca90e40ed14b83e}
      \field{labelnamesource}{author}
      \field{labeltitlesource}{title}
      \field{journaltitle}{\mnras}
      \field{month}{8}
      \field{title}{{Modelling feedback from stars and black holes in galaxy mergers}}
      \field{volume}{361}
      \field{year}{2005}
      \field{pages}{776\bibrangedash 794}
      \range{pages}{19}
      \verb{doi}
      \verb 10.1111/j.1365-2966.2005.09238.x
      \endverb
      \verb{eprint}
      \verb astro-ph/0411108
      \endverb
      \keyw{methods: numerical,galaxies: active,galaxies: interactions,galaxies: starburst,galaxies: structure}
    \endentry
    \entry{2005Natur.435..629S}{article}{}
      \name{author}{17}{}{%
        {{hash=0ef85848ecf64b63065e7d36351e48f4}{%
           family={{Springel}},
           familyi={S\bibinitperiod},
           given={V.},
           giveni={V\bibinitperiod}}}%
        {{hash=abcf743541bcfa11c3864021dc10c279}{%
           family={{White}},
           familyi={W\bibinitperiod},
           given={S.\bibnamedelimi D.\bibnamedelimi M.},
           giveni={S\bibinitperiod\bibinitdelim D\bibinitperiod\bibinitdelim M\bibinitperiod}}}%
        {{hash=bb1ab61d28c03aa08d44082bdc41aef5}{%
           family={{Jenkins}},
           familyi={J\bibinitperiod},
           given={A.},
           giveni={A\bibinitperiod}}}%
        {{hash=ec4d64fb832a8dc6453cbd14188a5b27}{%
           family={{Frenk}},
           familyi={F\bibinitperiod},
           given={C.\bibnamedelimi S.},
           giveni={C\bibinitperiod\bibinitdelim S\bibinitperiod}}}%
        {{hash=6b517fdbec59fd8f785f7ababcd23fc9}{%
           family={{Yoshida}},
           familyi={Y\bibinitperiod},
           given={N.},
           giveni={N\bibinitperiod}}}%
        {{hash=f25d2299651d8d644b6e27f50ea1fe77}{%
           family={{Gao}},
           familyi={G\bibinitperiod},
           given={L.},
           giveni={L\bibinitperiod}}}%
        {{hash=a79c110b752c2d25a0fcf559e67170a1}{%
           family={{Navarro}},
           familyi={N\bibinitperiod},
           given={J.},
           giveni={J\bibinitperiod}}}%
        {{hash=bbb05e166098153e2ad6355ed51afa4c}{%
           family={{Thacker}},
           familyi={T\bibinitperiod},
           given={R.},
           giveni={R\bibinitperiod}}}%
        {{hash=023bb5af2bd72b5661b062bdc8c80e89}{%
           family={{Croton}},
           familyi={C\bibinitperiod},
           given={D.},
           giveni={D\bibinitperiod}}}%
        {{hash=a053e0112a585080036f036b8915e7a0}{%
           family={{Helly}},
           familyi={H\bibinitperiod},
           given={J.},
           giveni={J\bibinitperiod}}}%
        {{hash=fdb25b48bf56f39c823bb4dc0733d757}{%
           family={{Peacock}},
           familyi={P\bibinitperiod},
           given={J.\bibnamedelimi A.},
           giveni={J\bibinitperiod\bibinitdelim A\bibinitperiod}}}%
        {{hash=e6704ec792c34e779ad19bdf8612d110}{%
           family={{Cole}},
           familyi={C\bibinitperiod},
           given={S.},
           giveni={S\bibinitperiod}}}%
        {{hash=2dbd0b71ac68ddca613b06761ae18a86}{%
           family={{Thomas}},
           familyi={T\bibinitperiod},
           given={P.},
           giveni={P\bibinitperiod}}}%
        {{hash=d4387b3bfc9cef45aacccd1dbf9598cd}{%
           family={{Couchman}},
           familyi={C\bibinitperiod},
           given={H.},
           giveni={H\bibinitperiod}}}%
        {{hash=6cddc68b68457206e956ae825835d18b}{%
           family={{Evrard}},
           familyi={E\bibinitperiod},
           given={A.},
           giveni={A\bibinitperiod}}}%
        {{hash=ec3b2687fafd5bc370f7fa269cf28ec6}{%
           family={{Colberg}},
           familyi={C\bibinitperiod},
           given={J.},
           giveni={J\bibinitperiod}}}%
        {{hash=5cdb148175a2fd88dc657e10eb1a36ed}{%
           family={{Pearce}},
           familyi={P\bibinitperiod},
           given={F.},
           giveni={F\bibinitperiod}}}%
      }
      \strng{namehash}{2f1654b4ba3c479b81cc56d9ce12c01e}
      \strng{fullhash}{363f0ed85b5502dd3d5b7a79feadad4f}
      \strng{authornamehash}{2f1654b4ba3c479b81cc56d9ce12c01e}
      \strng{authorfullhash}{363f0ed85b5502dd3d5b7a79feadad4f}
      \field{sortinit}{S}
      \field{sortinithash}{3c1547c63380458f8ca90e40ed14b83e}
      \field{labelnamesource}{author}
      \field{labeltitlesource}{title}
      \field{journaltitle}{\nat}
      \field{month}{6}
      \field{title}{{Simulations of the formation, evolution and clustering of galaxies and quasars}}
      \field{volume}{435}
      \field{year}{2005}
      \field{pages}{629\bibrangedash 636}
      \range{pages}{8}
      \verb{doi}
      \verb 10.1038/nature03597
      \endverb
      \verb{eprint}
      \verb astro-ph/0504097
      \endverb
    \endentry
    \entry{2016A&ARv..24...10T}{article}{}
      \name{author}{1}{}{%
        {{hash=5a8c8c488eef88ef4490419b4e6d5198}{%
           family={{Tadhunter}},
           familyi={T\bibinitperiod},
           given={C.},
           giveni={C\bibinitperiod}}}%
      }
      \strng{namehash}{5a8c8c488eef88ef4490419b4e6d5198}
      \strng{fullhash}{5a8c8c488eef88ef4490419b4e6d5198}
      \strng{authornamehash}{5a8c8c488eef88ef4490419b4e6d5198}
      \strng{authorfullhash}{5a8c8c488eef88ef4490419b4e6d5198}
      \field{sortinit}{T}
      \field{sortinithash}{2e5c2f51f7fa2d957f3206819bf86dc3}
      \field{labelnamesource}{author}
      \field{labeltitlesource}{title}
      \field{eid}{10}
      \field{eprinttype}{arXiv}
      \field{journaltitle}{\aapr}
      \field{month}{6}
      \field{title}{{Radio AGN in the local universe: unification, triggering and evolution}}
      \field{volume}{24}
      \field{year}{2016}
      \field{pages}{10}
      \range{pages}{1}
      \verb{doi}
      \verb 10.1007/s00159-016-0094-x
      \endverb
      \verb{eprint}
      \verb 1605.08773
      \endverb
      \keyw{Galaxies:active,Galaxies:jets,Galaxies:evolution}
    \endentry
    \entry{2016AN....337..410T}{article}{}
      \name{author}{1}{}{%
        {{hash=bd83509fe6c70d4bea2c3a66e2c0b2d0}{%
           family={{Tombesi}},
           familyi={T\bibinitperiod},
           given={F.},
           giveni={F\bibinitperiod}}}%
      }
      \strng{namehash}{bd83509fe6c70d4bea2c3a66e2c0b2d0}
      \strng{fullhash}{bd83509fe6c70d4bea2c3a66e2c0b2d0}
      \strng{authornamehash}{bd83509fe6c70d4bea2c3a66e2c0b2d0}
      \strng{authorfullhash}{bd83509fe6c70d4bea2c3a66e2c0b2d0}
      \field{sortinit}{T}
      \field{sortinithash}{2e5c2f51f7fa2d957f3206819bf86dc3}
      \field{labelnamesource}{author}
      \field{labeltitlesource}{title}
      \field{eprintclass}{astro-ph.HE}
      \field{eprinttype}{arXiv}
      \field{journaltitle}{Astronomische Nachrichten}
      \field{month}{5}
      \field{title}{{Accretion disk winds in active galactic nuclei: X-ray observations, models, and feedback}}
      \field{volume}{337}
      \field{year}{2016}
      \field{pages}{410}
      \range{pages}{1}
      \verb{doi}
      \verb 10.1002/asna.201612322
      \endverb
      \verb{eprint}
      \verb 1603.01235
      \endverb
      \keyw{accretion,accretion disks,black hole physics,galaxies: active,techniques: spectroscopic,X-rays: galaxies}
    \endentry
  \endsortlist
\endrefsection
\endinput

