Published December 19, 2022 | Version v1
Journal article Open

Evolution of the post merger remnants from the coalescence of oxygen-neon and carbon-oxygen white dwarf pairs

Authors/Creators

  • 1. Yunnan observatories, Chinese Academy of Sciences
  • 2. Research School of Astronomy and Astrophysics, The Australian National University
  • 3. Physics Department and Tsinghua Center for Astrophysics, Tsinghua University

Description

Inlists and initial models for simulating post-merger evolution of ONe WD + CO WD pairs.

Folder  includes initial models of  merger remnants and and inlists for calculating their post merger evolution, and the corresponding nuclear reaction network and opacity tables.

Folder named "fiducial_models"  includes initial models (after energy injection)   of  ONe+CO WD and ONe+HeCO WD merger remnants (including by considering different initial entropy profiles and nuclear reaction networks). Folder named "rotating _models" includes ONe+CO WD merger remnants with differential rotational velocities. Folder named "src" includes "run_star_extras.f90", in which different wind mass-loss prescriptions and stopping conditions can be setted.

Files

post_merger_evolution.zip

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