Figure 4 from The Fe Line Flux Ratio as a Diagnostic of the Maximum Temperature and the White Dwarf Mass of Cataclysmic Variables

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The Fe Line Flux Ratio as a Diagnostic of the Maximum Temperature and the White Dwarf Mass of Cataclysmic Variables

Authors: Xiao-jie Xu, Zhuo-li Yu, and Xiang-dong Li

2019 The Astrophysical Journal 878 53.

Provider: AAS Journals

Caption: Figure 4.

Left panel: M_WD derived from I_7.0/I_6.7 vs. dynamically determined M_WD. Right panel: M_WD derived from T_max vs. dynamically determined M_WD. The black (red) data points represent IPs (non-mCVs). The solid diagonal lines in both panels show a 1:1 relation for the M_WD values. The dashed lines show the best linear fit to the distribution (see Section 4.2 for details).

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