Inlists for paper: Stripped-Envelope Stars in Different Metallicity Environments I. Evolutionary Phases, Classification and Populations
Creators
- 1. Institute of Astrophysics, FORTH, Dept. of Physics, University of Crete, Voutes, University Campus, GR-71003 Heraklion, Greece
- 2. Argelander-Institut für Astronomie, Universität Bonn, Auf dem Hügel 71, 53121 Bonn, Germany
- 3. Institut für Physik und Astronomie, Universität Potsdam, Karl-Liebknecht-Str. 24/25, 14476 Potsdam, Germany
- 4. Institut d'Astrophysique de Paris, CNRS-Sorbonne Université, 98 bis boulevard Arago, F-75014 Paris, France
- 5. Department of Physics and Astronomy, Seoul National University, Gwanak-gu, Seoul, 151-742, Republic of Korea
Description
MESA input files for the models presented in the paper "Stripped-Envelope Stars in Different Metallicity Environments I. Evolutionary Phases, Classification and Populations".
The files included here can reproduce both the stellar models discussed in the paper (he_star_model.zip), as well as the initial helium star models (initial_model.zip). Some models used different numerical parameters to achieve convergence to core collapse. A table (MESA_params.dat) is included here with the specific models that have parameters that differ from the standard ones, and the value used for the parameters used in these models. To reproduce a model from this list, the parameters must be changed in the inlist_project file contained in he_star_model.zip.
Also included is a table (lifetimes.dat) containing values of different parameters used in each simulation, as well as the data obtained from these models, used to create Figs. 4 and 5.