mirror of
https://asciireactor.com/otho/phy-4660.git
synced 2024-12-05 02:35:05 +00:00
586 lines
22 KiB
Plaintext
586 lines
22 KiB
Plaintext
|
% $ 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
|
||
|
|