collaborators

5 papers

astro-ph.GA2025

Handy Relation Between Binary Black Hole Merger Times and Host Galaxy Properties

Kelly Holley-Bockelmann, Fazeel Khan, Isaiah Williams +6

Over the past 15 years, the evidence has clearly demonstrated that massive black hole (MBH) binary merger timescales depend strongly on the structural and kinematic properties of t…

astro-ph.GA2025

Intermediate Mass Ratio Inspirals in Milky Way Galaxies

Jillian Bellovary, Yuantong Luo, Thomas Quinn +3

A consequence of a non-zero occupation fraction of massive black holes (MBHs) in dwarf galaxies is that these MBHs can become residents of larger galaxy halos via hierarchical merg…

astro-ph.GA2025

Emission Line Diagnostics for IMBHs in Dwarf Galaxies: Accounting for BH Seeding and ULX Excitation

Chris T. Richardson, Jordan Wels, Kristen Garofali +13

Dwarf AGN serve as the ideal systems for identifying intermediate mass black holes (IMBHs) down to the most elusive regimes (). However, the ubiquitousl…

astro-ph.GA2025

Little Red Dots are Tidal Disruption Events in Runaway-Collapsing Clusters

Jillian Bellovary

I hypothesize a physical explanation for the "Little Red Dots" (LRDs) discovered by the James Webb Space Telescope (JWST). The first star formation in the universe occurs in dense…

astro-ph.GA2024

An Enhanced Massive Black Hole Occupation Fraction Predicted in Cluster Dwarf Galaxies

Michael Tremmel, Angelo Ricarte, Priyamvada Natarajan +3

The occupation fraction of massive black holes (MBHs) in dwarf galaxies offers interesting insights into initial black hole seeding mechanisms and their mass assembly history, thou…