“…It is fragmented into a chain of cores that are in the early evolutionary stages of low-mass star formation (Figure 1(b)). These include three prestellar cores, namely, Miz-8b, Miz-2, and HGBS-1 (Mizuno et al 1994;Marsh et al 2016); two class 0/I protostellar cores, IRAS 04166+2706 and IRAS 04169+2702 (Ohashi et al 1997;Tafalla et al 2010;Takakuwa et al 2018); and one evolved object, J04194148+2716070, classified as a class II T Tauri star (Davis et al 2010). We hereafter refer to IRAS 04166+2706 and IRAS 04169+2702 as K01466 and K04169, respectively (see Kenyon et al 1990Kenyon et al , 1993, adopting the core nomenclature of Bracco et al (2017).…”