Minimum gas mass accreted by spinning intermediate-mass black holes in stellar clusters. Kritos, K., Reali, L., Gerosa, D., & Berti, E. arXiv, September, 2024.
doi  bibtex   
@article{2024arXiv240915439K,
	adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	adsurl = {https://ui.adsabs.harvard.edu/abs/2024arXiv240915439K},
	archiveprefix = {arXiv},
	author = {{Kritos}, Konstantinos and {Reali}, Luca and {Gerosa}, Davide and {Berti}, Emanuele},
	doi = {10.48550/arXiv.2409.15439},
	eid = {arXiv:2409.15439},
	eprint = {2409.15439},
	journal = {arXiv},
	keywords = {Astrophysics - High Energy Astrophysical Phenomena, General Relativity and Quantum Cosmology},
	month = sep,
	pages = {arXiv:2409.15439},
	primaryclass = {astro-ph.HE},
	title = {{Minimum gas mass accreted by spinning intermediate-mass black holes in stellar clusters}},
	year = 2024,
	bdsk-url-1 = {https://doi.org/10.48550/arXiv.2409.15439}}

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