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On the Impact of Helium Content on the RR Lyrae Distance Scale

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Academic year: 2020

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Figure

Figure 1. Hertzsprung –Russell diagrams of low-mass helium burning stellar structures
Figure 2 shows the predicted optical /NIR PL distribution for five bands (R, I, J, H, K ) and for three different metal abundances: Z =0.0001 (left), Z=0.001 (middle), and Z=
Figure 3. Top: predicted (fundamentals plus first overtones) B-band mean magnitude metallicity (M B –[ Fe H ] ) relation

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