All Tables

Table 2: The coefficients a_i and b_i in Eq. (1).
Table 3: Absolute B, V, I magnitudes of Cepheids in open clusters.
Table 4: Absolute B, V, I magnitudes of Cepheids with distances from Gieren et al. (1998) ( $^{\ast }$ cf. notes in Table 3).
Table 5: Galactic P-L relations by different authors. The coefficients a and b are given for a P-L relation of the form $M=a(\log P -1)+b$ .
Table 6: The Distance Modulus of LMC independent of the P-L relation of Cepheids.
Table 7: The sensitivity of the P-L slope from the Tables 3 and 4 data to assumptions on reddening and broad-band effects ("Corr'' refers to ${E(B-V)_{{\rm corr}}}$ from Eq. (2); "FS'' refers to the ${E(B-V)_{{\rm FS}}}$ in the Fernie system).