Astronomy-General
Published April 7, 2022 | Version v1
Journal article Open

Formation of black holes in the pair-instability mass gap: Hydrodynamical simulation of a head-on massive star collision

Authors/Creators

  • 1. University of Padova
  • 2. Center for Astrophysics | Harvard & Smithsonian

Description

Input files and last simulation output for the paper:

Formation of black holes in the pair-instability mass gap: Hydrodynamical simulation of a head-on massive star collision
 

The compressed archive Input_files.tar.gz contains the input files to run the hydrodynamical simulation with the SPH code StarSmasher (Gaburov et al., 2010). WARNING: the StarSmasher file initialize_parent.f has to be slightly modified to read the PARSEC tables provided here.

The compressed archive Last_output.tar.gz contains the last output of the SPH simulation.

Files

Files (110.2 MB)

Name Size
md5:44000050a383dad3b5b97e809b9c0903
190.9 kB Download
md5:e1d424c2f666b8e7b57a74fb967a3c23
110.0 MB Download

Additional details

Funding

European Commission
DEMOBLACK - Demography of black hole binaries in the era of gravitational wave astronomy 770017