Outliers from the black hole-stellar mass scaling relation arise from distinct channels of enhanced mergers with super-Eddington growth, gravitational recoils after mergers, environmental stellar mass loss, and quiescent histories.
M., Ferrarese, L., Gilbert, K
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Recovers individual f virial factors from dynamical modeling plus RM data and reports evidence for correlation of log f with black hole mass plus marginal links to BLR thickness, inclination, and line shape.
Expanded sample yields marginal evidence that f correlates with log10(FWHM/σ) of the broad Hβ line, consistent with earlier results and potentially enabling empirical f estimates.
citing papers explorer
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Overmassive and Undermassive Massive Black Holes: The Role of Environment and Gravitational-Wave Recoils
Outliers from the black hole-stellar mass scaling relation arise from distinct channels of enhanced mergers with super-Eddington growth, gravitational recoils after mergers, environmental stellar mass loss, and quiescent histories.
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What Does the Virial Coefficient of the \Hb Broad-Line Region Depend On?
Recovers individual f virial factors from dynamical modeling plus RM data and reports evidence for correlation of log f with black hole mass plus marginal links to BLR thickness, inclination, and line shape.
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Can BLR line profile shape improve single-epoch black hole mass estimates?
Expanded sample yields marginal evidence that f correlates with log10(FWHM/σ) of the broad Hβ line, consistent with earlier results and potentially enabling empirical f estimates.