collaborators

5 papers

astro-ph.GA2026

Charting the Galactic Underworld I: Comprehensive simulations of the kinematics, rates, and demographics of Milky Way black holes

Tom Wagg, Katelyn Breivik, Adrian M. Price-Whelan +3

With upcoming data from Roman, Gaia DR4, and spectroscopic surveys, we will soon have an unprecedented dataset of Milky Way black holes (BHs) to constrain their formation and evolu…

astro-ph.HE2026

Twin Peaks: Resolving Features in the Binary Black Hole Mass Function with COSMIC-METISSE

Duncan B. Maclean, Poojan Agrawal, Katelyn Breivik +5

Gravitational waves from inspiraling binary black holes (BBHs) provide insights into the lives and deaths of massive stars. Population synthesis allows us to model these binaries t…

astro-ph.HE2026

Unraveling the Origin of Unequal Mass Gravitational Wave Events: Insights from a Galactic High Mass X-ray Binary

Neev Shah, Mathieu Renzo, Koushik Sen +2

The catalog of Gravitational Wave (GW) events is rapidly growing, providing key insights into the evolution of massive binaries and compact object formation. However, a key challen…

astro-ph.SR2025

Stellar ejection velocities from the binary supernova scenario: A comparison across population synthesis codes

Tom Wagg, David D. Hendriks, Mathieu Renzo +1

The vast majority of binary systems are disrupted at the moment of the first supernova, resulting in an unbound compact object and companion star. These ejected companion stars con…

astro-ph.SR2025

Delayed and Displaced: The Impact of Binary Interactions on Core-collapse SN Feedback

Tom Wagg, Julianne J. Dalcanton, Mathieu Renzo +7

Core-collapse supernova feedback models in hydrodynamical simulations typically assume that all stars evolve as single stars. However, the majority of massive stars are formed in b…