Three-component modelling of C-rich AGB-star winds V. – dataset

The provided data include all parameter files, binary output files, and log files that are the basis for the publication in MNRAS. The file 'file_listing.txt' contains a complete list of files and directories in all gzipped tar files. Each individual gzipped tar file is formatted as follows: Mm.m_Ll.ll_Ttttt_CtOc.cc.tar.gz where m.m :: the assumed mass of the model, in solar masses l.ll :: The assumed luminosity, in log10(solar luminosities) tttt :: The effective temperature of the star, in Kelvin. c.cc :: The carbon-to-oxygen excess, in log10(n_C/n_H-n_O/n_H)+12 The contents vary according to the model, but here is the general directory structure: nodr/ :: non-drift / PC models drift/ :: drift models nodr/init drift/init :: Initial model files created using John Connor. File suffixes are the following: .par :: Plain-text parameter file that contains all parameters that are different from the respective default value in the model. Consequently, to see all used parameters it is necessary to look in the log file (see below). .bin :: Binary file that contains converged models. Each model is stored in two versions, first the previous time step and then the current time step (both are needed to restart model calculations at that time step). The initial model file only contains one model; where the previous time step data are the same as the current time step data. The format of this file is explained below. Note! These files can get pretty large and are therefore only available for a smaller number of the models here. Please ask the corresponding author for the missing files should the need appear. .log :: Plain-text log file that shows the used model parameters and a number of key properties for each converged model. The encoding of this file is UTF-8. .inf :: Plain-text secondary log file that contains the header of the [primary] log file as well as timing information. .tpb :: Secondary binary file that contains a number of properties specified at the outer boundary, typically for each consecutive time step. .lis :: Plain-text file with the iteration history. Available for some files. .liv :: Plain-text file with values specified for a number of properties at each gridpoint. Available for a smaller number of files. .inp :: Plain-text file that is used to launch a model; some are still there. .eps :: Encapsulated PostScript files created by John Connor when calculating the initial model. Model evolution structure - file endings before the suffix: _rlx :: Files related to relaxing the T-800 calculations on the initial model created by John Connor. _exp :: Files related to expanding the initially compact model to using the full radial domain. _fix :: Files related to the intermediate stage where calculations are changed from expansion to outflow. _out :: Files related to the outflow stage of the calculations; this is what you want to look at to see the wind evolution. Results in the paper are calculated using these data. Note! Some outflow stage calculations continue the evolution of the previous set of files. The underlying reason for continued calculations is typically that the calculated time interval is too short. Such files are typically given the extension '_cont.lin_out', '_cont2.lin_out', etc. Load files: Two tools are provided here that can load the binary data files using the Interactive Data Language (IDL): sc_load_bin (for files with the suffix '.bin'): Loads the full content of a T-800 binary file and returns a structure with the data. sc_load_tpb (for files with the suffix '.tpb'): Loads the full content of a T-800 'tpb' binary file and returns a structure with the data. Note! Due to the way models run on clusters, this file is sometimes incomplete; this happens when the model code T-800 is stopped as the cluster-specific walltime is reached. If this is the case, it is necessary to use the binary file instead, where data are saved typically every 20:th time step. Alternative tools for use with Python and Julia could be considered for writing, but where not yet available when this dataset was made public. Please contact the corresponding author for a current status on this issue.