activity
20172021
most citedFormation of Double Neutron Star Systems

698 citations · 773 across the 4 of their papers we have counts for

collaborators

7 papers

astro-ph.SR202154 cited

A Catalogue of Potential Post Common Envelope Binaries

Matthias U. Kruckow, Patrick G. Neunteufel, Rosanne Di Stefano +2

We present a catalogue containing 839 candidate post common envelope systems. Common envelope evolution is very important in stellar astrophysics, particularly in the context of ve…

astro-ph.SR202013 cited

Predicted spatial and velocity distributions of ejected companion stars of helium accretion-induced thermonuclear supernovae

P. Neunteufel, M. Kruckow, S. Geier +1

Thermonuclear supernovae (SNe), a subset of which are the highly important SNe Type\,Ia, remain one of the more poorly understood phenomena known to modern astrophysics. In recent…

astro-ph.SR2020

Masses of double neutron star mergers

Matthias U. Kruckow

Aims. The mass discrepancy between the observed population of double neutron star binaries by radio pulsar observations and gravitational-wave observation requires an explanation.…

astro-ph.SR20198 cited

An Empirical Fit for Viscoelastic Simulations of Tertiary Tides

Yan Gao, Silvia Toonen, Evgeni Grishin +2

Tertiary tides (TTs), or the continuous tidal distortion of the tertiary in a hierarchical triple system, can extract energy from the inner binary, inducing within it a proclivity…

astro-ph.SR2018

The interaction of core-collapse supernova ejecta with a stellar companion

Zheng-Wei Liu, T. M. Tauris, F. K. Roepke +4

The progenitors of many core-collapse supernovae (CCSNe) are expected to be in binary systems. By performing a series of three-dimensional hydrodynamical simulations, we investigat…

astro-ph.HE2018

PSR J17552550: A young radio pulsar with a massive, compact companion

C. Ng, M. U. Kruckow, T. M. Tauris +9

Radio pulsars found in binary systems with short orbital periods are usually fast spinning as a consequence of recycling via mass transfer from their companion stars; this process…