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Binarity as the Solution to the Stellar Evolution Enigma Posed by NGC 6791
2017 The Astrophysical Journal Letters 841
Caption: Figure 3.
Same as Figure 2, but for the case in which CE resumes at 1 R⊙. Here, green, red, and blue solid lines correspond to models with masses of 0.34863, 0.37084, and 0.40973 M⊙, respectively.
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