PALL
发表于 2025-3-23 20:58:12
http://reply.papertrans.cn/39/3883/388240/388240_13.png
错事
发表于 2025-3-23 23:57:39
Interpersonal and Social Dynamics,e present preliminary results from a class of tidal disruption events that until now have not been considered in which the disruption-flare-disk sequence develops promptly. These tidal disruption events are from ultra-close encounters between main-sequence stars and intermediate mass black holes.
艺术
发表于 2025-3-24 03:23:09
Yves Dauvilliers,Giuseppe Plazziion of supermassive black holes from their host galaxies. We also discuss possible mechanisms that would make superkicks less likely to occur in astrophysical binaries and thus explain why most, if not all, galaxies observed in this context appear to harbor a black hole at their center.
Mere仅仅
发表于 2025-3-24 09:42:11
http://reply.papertrans.cn/39/3883/388240/388240_16.png
入会
发表于 2025-3-24 12:10:53
http://reply.papertrans.cn/39/3883/388240/388240_17.png
华而不实
发表于 2025-3-24 18:55:56
Gravitational Recoil and Astrophysical Impact,ion of supermassive black holes from their host galaxies. We also discuss possible mechanisms that would make superkicks less likely to occur in astrophysical binaries and thus explain why most, if not all, galaxies observed in this context appear to harbor a black hole at their center.
你敢命令
发表于 2025-3-24 22:27:07
http://reply.papertrans.cn/39/3883/388240/388240_19.png
Ganglion-Cyst
发表于 2025-3-25 01:33:07
https://doi.org/10.1007/978-1-4684-1869-9he parametric, turbulent instability of scalar fields on a background which includes a gravitational QNM, and the shifts to the QNM frequencies of Kerr when the black hole is weakly charged. This method may be of use in studies of black holes which are deformed by external fields or are solutions to alternative theories of gravity.
剧本
发表于 2025-3-25 06:24:46
http://reply.papertrans.cn/39/3883/388240/388240_21.png
蜈蚣
发表于 2025-3-25 10:21:43
http://reply.papertrans.cn/39/3883/388240/388240_22.png