The same assumptions as in Fig. 17. The dashed curves represent the error estimates by these authors. The red curves represents our determination of star #2 with c_K = 0.12 kpc^-1. The red curves are within the error limits quoted by Indebetouw et al. (2005). This is remarkable in view of the large difference in the E(J − K_s)/A_Ks and E(H − K_s)/A_Ks between our result for star #2 (which probes the outer regions of the B 335 globule plus diffuse clouds behind the globule) and the results of Indebetouw et al. (2005).