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Data for: "Toward a Comprehensive Grid of Cepheid Models with MESA. IV. Modest Effects of Rotation on Blue Loops"

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Zenodo2026-05-04 更新2026-05-26 收录
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Resources related to a paper "Toward a Comprehensive Grid of Cepheid Models with MESA. IV. Modest Effects of Rotation on Blue Loops" submitted for publication in Astrophysics Journal Supplement Series. All evolutionary tracks computed with Modules for Experiments in Stellar Astrophysics, MESA version r21.12.1, SDK version: 21.4.1 Evolutionary tracks associated with the paper: gzipped tar archives named as tracks_O00_ML4h_RA.tgz, tracks_O14_ML4h_RA.tgz, etc. Each archive contains tracks from dataset identified in file name, see Tab. 1 in the associated paper. Content of the files is described in Tab. 2 of the associated paper and in tracks_columns.txt. Naming scheme of the specific evolutionary tracks is the followinghistory.dat_SET_WR.RR_M.M_Z.ZZZZ_Y.YYYY, whereSET is a model set identifier, e.g., O00_ML4h_RAWR.RR is initial rotation rate, e.g., W0.50, means $W_0=0.50$Z.ZZZZ is metal mass fraction, e.g., 0.0060Y.YYYY is helium mass faction, e.g., 0.2575 Inlists associated with the paper (one per each data set listed in Table 1 of the paper; 9 inlists in total), e.g., inlist_project_O24_ML4h_RA_W050_5.0_0.0020_0.2515 where O24_ML4h_RA identifies a model set, followed by initial rotation rate (W050), initial mass (5.0), metal and helium content (0.0020_0.2515). For specific models within a given model set, inlist controls that are varied are: new_omega_div_omega_crit , initial_mass, new_y, new_z, Zbase Full version of Table 4: Tab4_online.txt - full version of Table 4 Tab4_online_columns.txt - description of columns Full version of Table 12 included in the Appendix of the paper: Tab12_online.txt - full version of Table 12 Tab12_online_columns.txt - description of columns

本数据集关联一篇已投稿至《天体物理学杂志增刊》(Astrophysics Journal Supplement Series)的论文《基于MESA构建完备造父变星模型网格 Ⅳ. 旋转对蓝循环的温和影响》(Toward a Comprehensive Grid of Cepheid Models with MESA. IV. Modest Effects of Rotation on Blue Loops)。 所有演化轨道均通过恒星天体物理学实验模块(Modules for Experiments in Stellar Astrophysics, MESA)版本r21.12.1计算得到,软件开发工具包(SDK)版本为21.4.1。 本论文关联的演化轨道: 以tracks_O00_ML4h_RA.tgz、tracks_O14_ML4h_RA.tgz等命名的gzip压缩tar归档文件。每个归档包含对应文件名标识的数据集轨道,详见关联论文中的表1。文件内容说明见关联论文的表2以及tracks_columns.txt文档。特定演化轨道的命名规则如下:history.dat_SET_WR.RR_M.M_Z.ZZZZ_Y.YYYY,其中:SET为模型集标识符(例如O00_ML4h_RA);WR.RR为初始旋转速率(例如W0.50,表示$W_0=0.50$);Z.ZZZZ为金属质量分数(例如0.0060);Y.YYYY为氦质量分数(例如0.2575)。 本论文关联的输入配置文件(inlist,共9个,对应论文表1中列出的每个数据集),示例如下: inlist_project_O24_ML4h_RA_W050_5.0_0.0020_0.2515 其中O24_ML4h_RA为模型集标识符,其后依次为初始旋转速率(W050)、初始质量(5.0)、金属丰度与氦丰度(0.0020_0.2515)。对于给定模型集中的特定模型,可通过inlist调整的参数包括:new_omega_div_omega_crit、initial_mass、new_y、new_z、Zbase。 表4完整版: Tab4_online.txt —— 表4完整内容 Tab4_online_columns.txt —— 列字段说明 论文附录中包含的表12完整版: Tab12_online.txt —— 表12完整内容 Tab12_online_columns.txt —— 列字段说明

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2026-03-26
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