The importance of nuclear star clusters for massive black hole growth and nuclear star formation in simulated low-mass galaxies
Observed low-mass galaxies with nuclear star clusters (NSCs) can host accreting massive black holes (MBH). We present simulations of dwarf galaxies (M-baryon similar to 0.6-2.4x10(8)M(circle dot)) at solar mass resolution (0.5M(circle dot)
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Partmann, C., Naab, T., Lahen, N., Rantala, A., Hirschmann, M., Hislop, J. M., Petersson, J., & Johansson, P. H. (2025). The importance of nuclear star clusters for massive black hole growth and nuclear star formation in simulated low-mass galaxies. Monthly Notices Of The Royal Astronomical Society, 537(2), 956–977. https://doi.org/10.1093/mnras/staf002
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