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adv_lab.bib
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adv_lab.bib
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@ARTICLE{2017ApJ...837..149G,
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author = {{Gaspari}, M. and {S{\c a}dowski}, A.},
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title = "{Unifying the Micro and Macro Properties of AGN Feeding and Feedback}",
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journal = {\apj},
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archivePrefix = "arXiv",
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eprint = {1701.07030},
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primaryClass = "astro-ph.HE",
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keywords = {black hole physics, galaxies: active, galaxies: clusters: intracluster medium, galaxies: groups: general, hydrodynamics, methods: numerical},
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year = 2017,
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month = mar,
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volume = 837,
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eid = {149},
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pages = {149},
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doi = {10.3847/1538-4357/aa61a3},
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adsurl = {http://adsabs.harvard.edu/abs/2017ApJ...837..149G},
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adsnote = {Provided by the SAO/NASA Astrophysics Data System}
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}
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@ARTICLE{2010A&A...523A..32K,
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author = {{Kroupa}, P. and {Famaey}, B. and {de Boer}, K.~S. and {Dabringhausen}, J. and
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{Pawlowski}, M.~S. and {Boily}, C.~M. and {Jerjen}, H. and {Forbes}, D. and
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{Hensler}, G. and {Metz}, M.},
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title = "{Local-Group tests of dark-matter concordance cosmology . Towards a new paradigm for structure formation}",
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journal = {\aap},
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archivePrefix = "arXiv",
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eprint = {1006.1647},
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keywords = {galaxies: dwarf, galaxies: evolution, gravitation, Local Group, dark matter, cosmology: theory},
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year = 2010,
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month = nov,
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volume = 523,
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eid = {A32},
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pages = {A32},
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doi = {10.1051/0004-6361/201014892},
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adsurl = {http://adsabs.harvard.edu/abs/2010A%26A...523A..32K},
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adsnote = {Provided by the SAO/NASA Astrophysics Data System}
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}
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@ARTICLE{2006astro.ph..8019L,
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@ARTICLE{2006astro.ph..8019L,
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author = {{Lemson}, G. and {Virgo Consortium}, t.},
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author = {{Lemson}, G. and {Virgo Consortium}, t.},
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title = "{Halo and Galaxy Formation Histories from the Millennium Simulation: Public release of a VO-oriented and SQL-queryable database for studying the evolution of galaxies in the LambdaCDM cosmogony}",
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title = "{Halo and Galaxy Formation Histories from the Millennium Simulation: Public release of a VO-oriented and SQL-queryable database for studying the evolution of galaxies in the LambdaCDM cosmogony}",
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\label{sec:cosmology}
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\label{sec:cosmology}
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\subsection{Millenium Simulation}
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\subsection{Millenium Simulation}
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The Millenium Simulation tests the \LCDM cosmology
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The Millenium Run and its following iterations are N-body simulations that predict the evolution of the matter in the universe. It is considered a (successful) test of the \LCDM cosmology.
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%─────────────
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%─────────────
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\section{Quasar Feedback Simulations}
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\section{Quasar Feedback Simulations}
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\label{sec:feedbacksims}
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\label{sec:feedbacksims}
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It is strongly believed by cosmologists that
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%─────────────
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%─────────────
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\section{Conclusion}
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\section{Conclusion}
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