Editing Galaxy formation and evolution (section)

====Supermassive black holes====

Simulation of supermassive black holes is also considered, numerically seeding them in dark matter haloes, due to their observation in many galaxies<ref name="MoranShahinyanSugarman2014">{{cite journal | last1 = Moran | first1 = Edward C. | last2 = Shahinyan | first2 = Karlen | last3 = Sugarman | first3 = Hannah R. | last4 = Vélez | first4 = Darik O. | last5 = Eracleous | first5 = Michael | title = Black Holes at the Centers of Nearby Dwarf Galaxies | journal = The Astronomical Journal | date = 13 November 2014 | volume = 148 | issue = 6 | page = 136 | eissn = 1538-3881 | doi = 10.1088/0004-6256/148/6/136 | pmid = | url = | arxiv = 1408.4451 | bibcode = 2014AJ....148..136M | s2cid = 118487176 }}</ref> and the impact of their mass on the mass density distribution. Their mass accretion rate is frequently modeled by the Bondi-Hoyle model.