Fig. 1
Three-colour image of B35A overlaid with SCUBA−2 850 μm density flux in units of mJy beam−1 (Reipurth & Friberg 2021); contours are in decreasing steps of 30% starting at 7.3 Jy beam−1. The composite is made from Spitzer IRAC 3.6 μm (blue), 4.5 μm (green), and Multiband Imaging Photometer for Spitzer (MIPS) 24.0 μm (red) bands (programme ID: 139, PI: N. J. Evans II). The white stars mark the positions of the AKARI and Spitzer c2d identified B35A sources. Connelley et al. (2008) and Reipurth & Friberg (2021) show the B35A sources to be multiplet systems totalling four or five objects.
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