activity
19982019
most citedFormation of Double Neutron Star Systems

698 citations · 1.1k across the 16 of their papers we have counts for

collaborators

16 papers

astro-ph.SR2019★ 30 cited

Evidence from high mass X-ray binaries that Galactic WR components of WR+O binaries end their life with a supernova explosion

D. Vanbeveren, N. Mennekens, E. P. J. van den Heuvel +1

Theoretical population number studies of binaries with at least one black hole (BH) component are obviously depending on whether or not BHs receive a (natal) kick during their form…

astro-ph.HE2018★ 21 cited

Binary neutron star formation and the origin of GW170817

K. Belczynski, T. Bulik, A. Olejak +11

The first neutron star-neutron star merger was detected in by LIGO/Virgo in a galaxy in which the majority of star formation was taking place a long time ago (11 Gyr). LIGO/Virgo e…

astro-ph.HE2017★ 20 cited

Formation of Double Neutron Stars, Millisecond Pulsars and Double Black Holes

Edward P. J. van den Heuvel

The 1982 model for the formation of the Hulse-Taylor binary radio pulsar PSR B1913+16 is described, which since has become the standard model for the formation of double neutron st…

astro-ph.HE2017★ 698 cited

Formation of Double Neutron Star Systems

T. M. Tauris, M. Kramer, P. C. C. Freire +11

Double neutron star (DNS) systems represent extreme physical objects and the endpoint of an exotic journey of stellar evolution and binary interactions. Large numbers of DNS system…

astro-ph2007★ 107 cited

Determination of the mass of the neutron star in SMC X-1, LMC X-4 and Cen X-3 with VLT/UVES

A. van der Meer, L. Kaper, M. H. van Kerkwijk +2

We present the results of a spectroscopic monitoring campaign of the OB-star companions to the eclipsing X-ray pulsars SMC X-1, LMC X-4 and Cen X-3. High-resolution optical spectra…

astro-ph2007★ 21 cited

Double Neutron Stars: Evidence For Two Different Neutron-Star Formation Mechanisms

E. P. J. van den Heuvel

Six of the eight double neutron stars known in the Galactic disk have low orbital eccentricities (< 0.27) indicating that their second-born neutron stars received only very small v…