field galaxies and their agns: nature versus nurture

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ID: 134456
2013
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Ranked #7 of 10 articles by views in saner 2019 - proceedings of the 2019 ieee 26th international conference on software analysis, evolution, and reengineering

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Abstract
This review attempts to present most recent findings related to the very controversial question of which processes guide the flow of gas to the galactic centers where the accretion and growth of supermassive black holes occurs. Also, we put this question in the context of influence of the environment (galaxy clusters versus field) onto these processes. [Projekat Ministarstva nauke Republike Srbije, br. 176021: Visible and Invisible Matter in Nearby Galaxies: Theory and Observations. The author acknowledges the financial support provided by the European Commission through project BELISSIMA (BELgrade Initiative for Space Science, Instrumentation and Modelling in Astrophysics, call FP7-REGPOT-2010-5, contract no. 256772]
Reference Key
m.2013serbianfield Use this key to autocite in the manuscript while using SciMatic Manuscript Manager or Thesis Manager
Authors ;Micic M.
Journal saner 2019 - proceedings of the 2019 ieee 26th international conference on software analysis, evolution, and reengineering
Year 2013
DOI
10.2298/SAJ1386001M
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