five

Three-component modelling of O-rich AGB star winds I. Effects of drift using forsterite – dataset

收藏
NIAID Data Ecosystem2026-05-01 收录
下载链接:
https://zenodo.org/record/8051248
下载链接
链接失效反馈
官方服务:
资源简介:
The data provided here include all parameter files, log files, and a set of the binary output files that are the basis for the publication in A&A. 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.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. The contents of the tar files 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 what parameters were actually used, it is      necessary to look in the log file (see below).  .bin :: Binary file that contains output of converged models. Each model is          stored in two versions, first the previous time step and then the      current time step (having access to the model code T-800, data of both      time steps 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.          We provide a tool to read this file, see below.          Note! These files can get pretty large and are therefore only        available for a smaller number of the models in the Zenodo dataset.        Please ask the corresponding author for the missing files is the        need should 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.      The encoding of this file is UTF-8.  .tpb :: Secondary binary file that contains a number of properties specified          at the outer boundary, typically for each consecutive time step.          We provide a tool to read this file, see below.  .lis :: Plain-text file with the iteration history. Unavailable here.  .liv :: Plain-text file with values specified for a number of properties at          each gridpoint. Unavailable here.  .inp :: Plain-text file that is used to launch a model; some are present.          This file is automatically generated by the tool that launches T-800      and is typically removed when T-800 launches. Unavailable here.  .eps :: Encapsulated PostScript file 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. Stored data in the binary files:  The binary files (suffix '.bin') contain the full radial structure in the  following 10 (PC models) or 11 (drift models) primary variables:    mr: radius    mm: integrated [gas] mass    md: gas density    mu: gas velocity    me: internal energy    mj: radiative energy    mh: radiative flux    n0: dust moment, forsterite (Fo)    nm: number density of magnesium atoms    ns: number density of silicon atoms    v0: dust velocity, forsterite (only drift models)  Other properties are derived from these primary variables using auxiliary code  that isn't part of this dataset. 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.
创建时间:
2023-06-19
5,000+
优质数据集
54 个
任务类型
进入经典数据集
二维码
社区交流群

面向社区/商业的数据集话题

二维码
科研交流群

面向高校/科研机构的开源数据集话题

数据驱动未来

携手共赢发展

商业合作