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Stellar Mass Distribution and Star Formation History of the Galactic Disk Revealed by Mono-age Stellar Populations from LAMOST

  • Authors: Maosheng Xiang, Jianrong Shi, Xiaowei Liu, Haibo Yuan, Bingqiu Chen, Yang Huang, Chun Wang, Yaqian Wu, Zhijia Tian, Zhiying Huo, Huawei Zhang, and Meng Zhang

2018 The Astrophysical Journal Supplement Series 237 33.

  • Provider: AAS Journals

Caption: Figure 11.

Left: ratios between the derived mean density within ﹩| Z| \lt 50﹩ pc from the mock data and the input mean stellar mass density within ﹩| Z| \lt 50﹩ pc (solid line) or the input midplane density (dashed line). Right: ratios between the derived and the model input surface mass density. For both the left and the right panels, the red symbol shows the result of the whole stellar population of 0–14 Gyr. The horizontal lines delineate the constant values of 1.0 and 1.2.

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