Which black hole formed first? Mass-ratio reversal in massive binary stars from gravitational-wave data. Mould, M., Gerosa, D., Broekgaarden, F. S., & Steinle, N. Monthly Notices of the Royal Astronomical Society, 517(2):2738-2745, December, 2022.
doi  bibtex   
@article{2022MNRAS.517.2738M,
	adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	adsurl = {https://ui.adsabs.harvard.edu/abs/2022MNRAS.517.2738M},
	archiveprefix = {arXiv},
	author = {{Mould}, Matthew and {Gerosa}, Davide and {Broekgaarden}, Floor S. and {Steinle}, Nathan},
	doi = {10.1093/mnras/stac2859},
	eprint = {2205.12329},
	journal = {Monthly Notices of the Royal Astronomical Society},
	keywords = {gravitational waves, black hole mergers, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Solar and Stellar Astrophysics, General Relativity and Quantum Cosmology},
	month = dec,
	number = {2},
	pages = {2738-2745},
	primaryclass = {astro-ph.HE},
	title = {{Which black hole formed first? Mass-ratio reversal in massive binary stars from gravitational-wave data}},
	volume = {517},
	year = 2022,
	bdsk-url-1 = {https://doi.org/10.1093/mnras/stac2859}}

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