Do Intermediate-Mass Black Holes Exist in Globular Clusters?
arXiv:1308.2869 · doi:10.1088/0004-637X/776/2/118
Abstract
The existence of intermediate-mass black holes (IMBHs) in globular clusters (GCs) remains a crucial problem. Searching IMBHs in GCs reveals a discrepancy between radio observations and dynamical modelings: the upper mass limits constrained by radio observations are systematically lower than that of dynamical modelings. One possibility for such a discrepancy is that, as we suggest in this work, there exist outflows in accretion flows. Our results indicate that, for most sources, current radio observations cannot rule out the possibility that IMBHs may exist in GCs. In addition, we adopt an \dot{M}-L_{R} relation to revisit this issue, which confirms the results obtained by the Fundamental Plane relation.
18 pages, 2 figures, accepted for publication in ApJ
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Cited by in corpus (10)
- Evidence for an intermediate-mass black hole in the globular cluster NGC 6624
- Observational Evidence for a Dark Side to NGC5128's Globular Cluster System
- MOCCA-SURVEY Database I: Is NGC 6535 a Dark Star Cluster Harboring an IMBH?
- Binary black hole growth by gas accretion in stellar clusters
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- Prospects for Revealing Intermediate-Mass Black Holes in NGC 1399 using SKA