P. Fouque et Wp. Gieren, COMPARISON OF THE OPEN CLUSTER AND SURFACE BRIGHTNESS DISTANCE SCALESFOR GALACTIC CLASSICAL CEPHEIDS, Astrophysical letters & communications, 31(1-6), 1995, pp. 243-250
We compare a new period-luminosity (PL) relation, derived by the ZAMS-
fitting method for 32 cluster and association Cepheids, to the best de
termined Baade-Wesselink (BW) PL relation for 100 stars. Eighteen star
s in common lead to conclude that BW and ZAMS-fitting distances can ag
ree within 0.1 mag, after proper allowance of possible systematic effe
cts.