% $ 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