The dark nemesis of galaxy formation: why hot haloes trigger black hole growth and bring star formation to an end. Bower, R. G., Schaye, J., Frenk, C. S., Theuns, T., Schaller, M., Crain, R. A., & McAlpine, S. Monthly Notices of the Royal Astronomical Society, 465(1):32–44, February, 2017.
The dark nemesis of galaxy formation: why hot haloes trigger black hole growth and bring star formation to an end [link]Paper  doi  abstract   bibtex   
Abstract. Galaxies fall into two clearly distinct types: ‘blue-sequence’ galaxies which are rapidly forming young stars, and ‘red-sequence’ galaxies in which s
@article{bower_dark_2017,
	title = {The dark nemesis of galaxy formation: why hot haloes trigger black hole growth and bring star formation to an end},
	volume = {465},
	issn = {0035-8711},
	shorttitle = {The dark nemesis of galaxy formation},
	url = {https://academic.oup.com/mnras/article/465/1/32/2417457},
	doi = {10.1093/mnras/stw2735},
	abstract = {Abstract.  Galaxies fall into two clearly distinct types: ‘blue-sequence’ galaxies which are rapidly forming young stars, and ‘red-sequence’ galaxies in which s},
	language = {en},
	number = {1},
	urldate = {2019-01-28},
	journal = {Monthly Notices of the Royal Astronomical Society},
	author = {Bower, Richard G. and Schaye, Joop and Frenk, Carlos S. and Theuns, Tom and Schaller, Matthieu and Crain, Robert A. and McAlpine, Stuart},
	month = feb,
	year = {2017},
	pages = {32--44},
}

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