collaborators

7 papers

astro-ph.GA2026

Supermassive black holes in six triaxial galaxies: Insights from SINFONI and MUSE observations

Sabine Thater, Avinash Chaturvedi, Davor Krajnovic +5

Dynamical modelling can be used to constrain the masses of central black holes; however, modelling massive galaxies is challenging due to their complexity. In this work, we report…

astro-ph.GA2026

How Overmassive Black Holes Formed at Cosmic Dawn

Muhammad A. Latif, Daniel J. Whalen, Sadegh Khochfar +1

Overmassive black hole galaxies (OBGs) at redshifts 10, or 450 Myr after the Big Bang, are one of the most puzzling discoveries by the James Webb Space Telescope to date b…

astro-ph.GA2026

Impact of subhalo dynamical friction heating on the formation of the first structures in the universe

Zhenyu Wu, Sadegh Khochfar, Muhammad A. Latif +2

We present a model for gas heating, driven by dynamical friction from orbiting subhalos within dark matter halos. Using data from the TNG50 simulation, we derive the subhalo mass f…

astro-ph.CO2025

Clustering effects on the Dark Siren determination of : A simulation study

Marios Kalomenopoulos, Riccardo Barbieri, Sadegh Khochfar +2

Gravitational waves (GWs) offer an alternative way to measure the Hubble parameter. The optimal technique, the ``bright siren'' approach, requires the identification of an electrom…

astro-ph.GA2025

Gaseous Dynamical Friction: a Numerical Study of Extended Perturbers

Ben Morton, Sadegh Khochfar, Jose Oñorbe

The process of momentum and energy transfer between a massive body and a background medium it is moving through is known as dynamical friction (DF). It is key to our understanding…

astro-ph.GA2025

Conditions for Super-Eddington Accretion onto the First Black Holes

Simone T. Gordon, Britton D. Smith, Sadegh Khochfar +1

Observations of supermassive black holes at high redshift challenge our understanding of the evolution of the first generation of black holes (BHs) in proto-galactic environments.…