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							| @ -1,3 +1,45 @@ | ||||
| 
 | ||||
| @ARTICLE{2017ApJ...837..149G, | ||||
|    author = {{Gaspari}, M. and {S{\c a}dowski}, A.}, | ||||
|     title = "{Unifying the Micro and Macro Properties of AGN Feeding and Feedback}", | ||||
|   journal = {\apj}, | ||||
| archivePrefix = "arXiv", | ||||
|    eprint = {1701.07030}, | ||||
|  primaryClass = "astro-ph.HE", | ||||
|  keywords = {black hole physics, galaxies: active, galaxies: clusters: intracluster medium, galaxies: groups: general, hydrodynamics, methods: numerical}, | ||||
|      year = 2017, | ||||
|     month = mar, | ||||
|    volume = 837, | ||||
|       eid = {149}, | ||||
|     pages = {149}, | ||||
|       doi = {10.3847/1538-4357/aa61a3}, | ||||
|    adsurl = {http://adsabs.harvard.edu/abs/2017ApJ...837..149G}, | ||||
|   adsnote = {Provided by the SAO/NASA Astrophysics Data System} | ||||
| } | ||||
| 
 | ||||
| 
 | ||||
| 
 | ||||
| @ARTICLE{2010A&A...523A..32K, | ||||
|    author = {{Kroupa}, P. and {Famaey}, B. and {de Boer}, K.~S. and {Dabringhausen}, J. and  | ||||
|   {Pawlowski}, M.~S. and {Boily}, C.~M. and {Jerjen}, H. and {Forbes}, D. and  | ||||
|   {Hensler}, G. and {Metz}, M.}, | ||||
|     title = "{Local-Group tests of dark-matter concordance cosmology . Towards a new paradigm for structure formation}", | ||||
|   journal = {\aap}, | ||||
| archivePrefix = "arXiv", | ||||
|    eprint = {1006.1647}, | ||||
|  keywords = {galaxies: dwarf, galaxies: evolution, gravitation, Local Group, dark matter, cosmology: theory}, | ||||
|      year = 2010, | ||||
|     month = nov, | ||||
|    volume = 523, | ||||
|       eid = {A32}, | ||||
|     pages = {A32}, | ||||
|       doi = {10.1051/0004-6361/201014892}, | ||||
|    adsurl = {http://adsabs.harvard.edu/abs/2010A%26A...523A..32K}, | ||||
|   adsnote = {Provided by the SAO/NASA Astrophysics Data System} | ||||
| } | ||||
| 
 | ||||
| 
 | ||||
| 
 | ||||
| @ARTICLE{2006astro.ph..8019L, | ||||
|    author = {{Lemson}, G. and {Virgo Consortium}, t.}, | ||||
|     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}", | ||||
|  | ||||
| @ -47,14 +47,14 @@ | ||||
|     \label{sec:cosmology} | ||||
| 
 | ||||
|     \subsection{Millenium Simulation} | ||||
|     The Millenium Simulation tests the \LCDM cosmology  | ||||
|     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. | ||||
| 
 | ||||
| 
 | ||||
| %───────────── | ||||
| \section{Quasar Feedback Simulations} | ||||
| \label{sec:feedbacksims} | ||||
| 
 | ||||
|      | ||||
|     It is strongly believed by cosmologists that  | ||||
| 
 | ||||
| %───────────── | ||||
| \section{Conclusion} | ||||
|  | ||||
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