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8 results for “MESA inlists”
Type Ia supernovae from non-accreting progenitors: data, python scripts and mesa inlists
<p>This release contains the inlists and final profiles described in: Antoniadis et al., "Type Ia supernovae from non-accreting progenitors" Mesa v. 10398</p>
MESA inlists for 'Revisiting the Red Giant Branch Hosts KOI-3886 and $\iota$ Draconis. Detailed Asteroseismic Modeling and Consolidated Stellar Parameters' by Campante et al.
<p>MESA inlists used in preparation of the paper 'Revisiting the Red Giant Branch Hosts KOI-3886 and $\iota$ Draconis. Detailed Asteroseismic Modeling and Consolidated Stellar Parameters' by Campante et al. Two folders are provided in the .zip file:</p> <ul> <li>TL_Pipeline — inlists (MESA release version 12115) used to build the grid of stellar models used in Sect. 4.1 of the paper.</li> <li>JO_Pipeline — inlists (MESA release version 12778) used to build both grids of stellar models used in Sect. 4.2 of the paper.</li> </ul>
Animation, MESA inlists, and post-processing package for "Is Betelgeuse really rotating? Synthetic ALMA observations of large-scale convection in 3D simulations of Red Supergiants"
<p>Videos, post-processing package for mock ALMA observations, MESA (r23.05.1 with mesasdk-x86_64-linux-23.7.3) inlists and history files, Jupyter notebook and data to reproduce figures of the paper "Is Betelgeuse really rotating? Synthetic ALMA observations of large-scale convection in 3D simulations of Red Supergiants".</p>
MESA inlists for: Type Ia Supernovae from the First Generation Stars
<p>MESA input files associated with the paper "Type Ia Supernovae from the First Generation Stars". This directory contains MESA inlists and run_star_extras.f used for calculations performed with MESA r12115. The MESASDK version is aarch64-macos-22.10.1. </p> <p> </p> <p>MESA simulations of Single Degnerate Channel for SNe Ia at zero metallicity. The Common Envelope Wind model (Meng,X & Podsiadlowski,Ph) is adopted.</p> <p>inlist1: Evove the 1st star (primary star)</p> <p>inlist2: mass point (Secondary star)</p> <p>inlist_project: Inputs for binary evolution</p> <p>run_binary_extras.f: The Common Envelope Wind model for WD accretion. </p>
MESA Inlists for: Barium Surface Abundances of Blue Straggler Stars in the Open Clusters NGC 7789 and M67
<p>These are the MESA v15140 inlists and Python script associated with the models presented in Nine et al. (2024). The files are as follows:</p> <p>inlist, inlist_start_header, inlist_to_end_core_h_burn_header, inlist_to_start_he_core_flash_header, inlist_to_end_core_he_burn_header, inlist_to_end_agb_header, inlist_to_wd_header: Pointer files to tell MESA which inlists to read for control, kappa, and PGStar commands.</p> <p>inlist_start, inlist_to_end_core_h_burn, inlist_to_start_he_core_flash, inlist_to_end_core_he_burn, inlist_to_end_agb, inlist_to_wd: MESA inlist files with control, kappa, and PGStar commands for each stage.</p> <p>turnoff_masses.py: a Python script that takes in the file inlist_start_base and rewrites it to create a starting model with the mass of a turnoff star in NGC 7789 (1.8 solar masses), NGC 6819 (1.5 solar masses), M67 (1.3 solar masses), and NGC 188 (1.1 solar masses). This starting model is then used in the following inlists to create AGB star models with these masses.</p> <p>inlist_start_base: The base starting inlist that turnoff_masses.py reads in and alters to create inlist_start.</p>
Magnetic braking with MESA evolutionary models in the single star and LMXB regimes (Gossage et al. 2023) - Inlists, source code, history files
<p>Associated MESA (r11701) inlists, source files (run_star_extras.f90 and run_binary_extras.f), and outputs (history files for single star models --but the same for binary star models is available upon request) used in producing models featured in <a href="https://ui.adsabs.harvard.edu/abs/2022arXiv221212037G/abstract">Gossage et al. 2023 - Magnetic braking with MESA evolutionary models in the single star and LMXB regimes</a>). README files are included, and please contact to alert me of any issues.</p>
MESA inlists for "Coping with loss: Stability of mass transfer from post-main-sequence donor stars"
<p>Binary model inlists for MESA, as used for the paper <a href="https://ui.adsabs.harvard.edu/abs/2023A%26A...669A..45T/abstract">Coping with loss: Stability of mass transfer from post-main-sequence donor stars</a> . The inlists provided here are pared-down, minimal working examples of the ones used in the publication. Due to the nature of the calculations, it was often needed to fine-tune inlists for specific systems by hand. For example, AGB models typically required the additional setting of <em>use_gold_tolerances = .false.</em></p> <p>These binary calculations start from a previously-evolved single star model for the donor stars. These can be found in the compressed folder titled "sstar_models_CWL.tar.xz". Please note that several parameters in the inlists will need to be adjusted accordingly, such as the configuration (initial orbit; mass ratio) of the binaries.</p> <p> </p> <p><strong>NOTE:</strong> to ensure that the mass-transfer calculation is fully conservative, add the following line to the <em>binary_controls</em> namelist in the <em>inlist_project</em> file:</p> <blockquote> <p>use_radiation_corrected_transfer_rate = .false.</p> </blockquote> <p>Further advice, code and/or files are available upon reasonable request to the authors (<a href="mailto:Karel.Temmink@ru.nl">contact: Karel Temmink</a>).</p>
Low-mass stellar models (MESA v15140 inlists)
<p>Low-mass stellar models (MESA v15140 inlists)</p>
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