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Fig. 5

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OMC-2 (upper panels) and LDN 1641N (lower panels) as seen in different surveys. Left panels: ALMA+IRAM-30 m integrated emission of N2H+ (1−0) at 4.5″. Central panels: CARMA-NRO integrated emission of C18 O (1−0) at 8″ (Suri et al. 2019). The white dotted line is the footprint of our ALMA+IRAM-30 m observations. Right panels: Herschel+Spitzer dust continuum at 36.2″ (Lombardi et al. 2014). The gold dotted line is the footprint of our ALMA+IRAM-30 m observations, while the white contours represent I(N2H+) > 5 K km s−1, twice as those in Fig. 1 to highlight the tight correspondence with the high column density material.

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