Color‐magnitude diagram for the stars in the NGC 2024 cluster (based on data from Meyer 1996). We also plot the isochrone for stars of age 0.3 Myr (D’Antona & Mazzitelli 1997) and the extinction vectors (Cohen et al. 1981) for a 1 M_⊙ star and a 0.1 M_⊙ star, assuming ﹩A_{V}=20﹩. Sources that lie within the unit gain contour of our OVRO mosaic (see Fig. 2) are indicated by filled circles, while open circles represent cluster members that lie outside the unit gain region.