The Influence of the Metal Mass Fraction Z, Age, and Mixing-length Parameter on the RGB Bump Magnitude for the M4 Cluster

The Influence of the Metal Mass Fraction Z, Age, and Mixing-length Parameter on the RGB Bump Magnitude for the M4 Cluster
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金属质量分数 Z、年龄和混合长度参数对 M4 团簇 RGB 凹凸大小的影响

DOI:
10.3847/1538-4357/aaecd3
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发表时间:
2018-12
影响因子:
4.9
通讯作者:
Xie Yi
Xie Yi
中科院分区:
物理与天体物理2区
文献类型:
--
作者:
Song Fen;Li Yan;Wu Tao;Pietrinferni Adriano;Poon Helen;Xie Yi

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我们使用现有的光度数据确定了M4(NGC 6121)的RGB凸起的位置,并测量了VRGBB(13.57 ± 0.04等)。根据观测到的[Fe/H],我们计算了梅萨模型中定标太阳成分的理论等时线
We identify the location of the RGB bump of M4 (NGC 6121) using the available photometric data, and measure VRGBB (∼13.57 ± 0.04 mag). According to the observed [Fe/H], we compute theoretical isochrones with the scaled-solar composition in the MESA model
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