Magnetic signatures in merger products
All template inlist files used to create the stellar models used in the 'Magnetic signatures in merger products' paper, as well as our additions to the 'run_star_extras.f90' file used to enable a nu_max-based stopping criterion. The single-star models were calculated based on the following inlist: single_inlist The mass-gain models were calculated based on the following inlists, executed in the order given here: merger_inlist_initial_ascend merger_inlist_merging_process merger_inlist_second_ascend The 'extras_check_model' function in the 'run_star_extras.f90' files of both model types was expanded via the custom numax stopping criterion found in the 'run_star_extras_addition.txt' file.
Authors
- Lukas Einramhof (ORCID: https://orcid.org/0009-0002-5619-0598)
- L. Bugnet (ORCID: https://orcid.org/0000-0003-0142-4000)
- Pierre Beck (ORCID: https://orcid.org/0000-0002-6532-5602)
- Lynn Buchele (ORCID: https://orcid.org/0000-0003-1666-4787)
- N. Muntean (ORCID: https://orcid.org/0009-0000-1750-8618)
- Bastien Liagre (ORCID: https://orcid.org/0009-0008-7869-7430)
- Debasish Dutta (ORCID: https://orcid.org/0009-0000-1383-8011)
- L. Barrault (ORCID: https://orcid.org/0009-0007-7748-900X)
Institutions
- Institute of Science and Technology Austria (AT)
- Universidad de La Laguna (ES)
- Université Paris Cité (FR)
- Instituto de Astrofísica de Canarias (ES)
Publication Details
- Journal
- Zenodo (CERN European Organization for Nuclear Research)
- Published
- 2026-10-14
- DOI
- https://doi.org/10.5281/zenodo.23364968
- Primary Topic
- Stellar, planetary, and galactic studies
- Type
- article
- Field-Weighted Citation Impact
- 0.00