Simulations indicate stellar collisions dominate intermediate-mass black hole formation across cluster types, with potential to explain local globular cluster candidates and predict wandering IMBHs in Milky Way-like galaxies.
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Uncertainties in stellar evolution and IMF lead to stellar mass errors of ~0.3 dex at z~0 and ~0.6 dex at z~2, plus ~0.4 mag uncertainty in K-band luminosity evolution per unit redshift.
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Seeds to success: growing heavy black holes in dense star clusters
Simulations indicate stellar collisions dominate intermediate-mass black hole formation across cluster types, with potential to explain local globular cluster candidates and predict wandering IMBHs in Milky Way-like galaxies.
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The propagation of uncertainties in stellar population synthesis modeling I: The relevance of uncertain aspects of stellar evolution and the IMF to the derived physical properties of galaxies
Uncertainties in stellar evolution and IMF lead to stellar mass errors of ~0.3 dex at z~0 and ~0.6 dex at z~2, plus ~0.4 mag uncertainty in K-band luminosity evolution per unit redshift.