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The Kleinmann–Low (KL) nebula in Orion, at a distance 415 pc (Menten et al. 2007; Kim et al. 2008; Kounkel et al. 2018), is the nearest HII region in which massive (M > 8 M⊙) stars are forming. The two most massive objects in this region, Source I (SrcI) and the Becklin–Neugebauer Object (BN), appear to be recoiling from one another at 35–40 km s−1 (Rodríguez et al. 2005; Gómez et al. 2008; Goddi et al.
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