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Stellar-mass binary black holes may have circumbinary disks if formed through common-envelope evolution or within gaseous environments. Disks can drive binaries into wider and more eccentric orbits, while gravitational waves harden and circularise th
Externí odkaz:
http://arxiv.org/abs/2407.03869
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters; Oct2024, Vol. 534 Issue 1, pL58-L64, 7p
