All Tables

Table 1: Basic parameters of the pulsation models and resulting effective temperatures at the edges for fundamental and first-overtone pulsation.
Table 2: Chemical compositions of the adopted evolutionary models.
Table 3: Luminosity $L_{\rm FBE}$ at the fundamental blue edge of the models with the labeled metal content and [ $\alpha$ /Fe] = 0.4, compared to the luminosity $L_{\rm IP}$ at the intersection between FOBE and FBE.
Table 4: Predicted PM_I, PM_J, PM_H, and PM_K relations for fundamental pulsators with iron content in the range of [Fe/H] = -2.6 to -0.7 and $P\le$ 8 days.
Table 5: PW relations for fundamental pulsators with iron content in the range of [Fe/H] = -2.6 to -0.7 and period $P\le$ 8 days.
Table 6: Galactic globular clusters with observed P2Cs.
Table 7: Mean intrinsic distance moduli (in magnitudes), as derived by the Wesenheit functions of BL Her and W Vir stars (the quantity Nis the number of averaged values).