activity
20022026
most citedThe Landscape of the Neutrino Mechanism of Core-Collapse Supernovae: Neutron Star and Black Hole Mass Functions, Explosion Energies and Nickel Yields

244 citations · 3.3k across the 56 of their papers we have counts for

collaborators

58 papers

astro-ph.HE2026

Quantifying the impact of relativistic precession on tidal disruption event light curves

Diego Calderón, Ondřej Pejcha, Brian D. Metzger +2

The tidal field of a black hole can turn a star into a gas stream whose orbit can precess, especially if the a black hole is rapidly spinning. In this work, we investigate the impa…

astro-ph.SR2025★ 6 cited

Two-Dimensional Radiation-Hydrodynamic Simulations of Luminous Red Novae

Anthony Kirilov, Diego Calderón, Ondřej Pejcha +1

Luminous Red Novae (LRNe) are transients associated with mass ejection during stellar mergers and common envelope evolution (CEE). LRNe have the potential to illuminate the poorly…

astro-ph.SR2025★ 2 cited

On the effects of radiation on mass transfer in binary stars

Jakub Cehula, Ondřej Pejcha

Mass transfer (MT) in binary systems is a common evolutionary process that can significantly affect the structure, evolution, and final fate of both stars. In modeling MT hydrodyna…

astro-ph.SR2024★ 6 cited

Journey to the center of the common envelope evolution. Inner dynamics of the post-dynamical inspiral

Damien Gagnier, Ondrej Pejcha

Three-dimensional hydrodynamical simulations of common envelope evolution are often terminated soon after the initial dynamical plunge of the companion transitions into a long-last…

astro-ph.SR2024★ 2 cited

Distinguishing between light curves of ellipsoidal variables with massive dark companions, contact binaries, and semidetached binaries using principal component analysis

Milan Pešta, Ondřej Pejcha

Photometric methods for identifying dark companion binaries - binary systems hosting quiescent black holes and neutron stars - operate by detecting ellipsoidal variations caused by…

astro-ph.SR2024

Driving asymmetric red supergiants winds with binary interactions

Camille Landri, Ondřej Pejcha

Massive stars in the red supergiant (RSG) phase are known to undergo strong mass loss through winds and observations indicate that a substantial part of this mass loss could be dri…