Detailed view of the Mon R2 center region, based on the same UKIRT WFCAM 2.12 μm S(1) line + continuum image as Fig. 1. The two CO outflows identified by Tafalla et al. (1997), Mon R2 N and CO −100, −40, are indicated, as well as the newly found outflows HOD07 7 and 10. The positions of the three dominant infrared sources, IRS 1–3 (Beckwith et al. 1976), are indicated in the overexposed central region of the Mon R2 cluster. The positions of many of the small reflection nebulae from Table 2 are indicated by squares.