Spin orientations of merging black holes formed from the evolution of stellar binaries. Gerosa, D., Berti, E., O'Shaughnessy, R., Belczynski, K., Kesden, M., Wysocki, D., & Gladysz, W. Physical Review D, 98(8):084036, October, 2018.
doi  bibtex   
@article{2018PhRvD..98h4036G,
	adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	adsurl = {https://ui.adsabs.harvard.edu/abs/2018PhRvD..98h4036G},
	archiveprefix = {arXiv},
	author = {{Gerosa}, Davide and {Berti}, Emanuele and {O'Shaughnessy}, Richard and {Belczynski}, Krzysztof and {Kesden}, Michael and {Wysocki}, Daniel and {Gladysz}, Wojciech},
	doi = {10.1103/PhysRevD.98.084036},
	eid = {084036},
	eprint = {1808.02491},
	journal = {Physical Review D},
	keywords = {Astrophysics - High Energy Astrophysical Phenomena, General Relativity and Quantum Cosmology},
	month = oct,
	number = {8},
	pages = {084036},
	primaryclass = {astro-ph.HE},
	title = {{Spin orientations of merging black holes formed from the evolution of stellar binaries}},
	volume = {98},
	year = 2018,
	Bdsk-Url-1 = {https://doi.org/10.1103/PhysRevD.98.084036}}

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