Fig. 8
Comparison of [OI] 63 μm and 63 μm continuum fluxes to those of jet and nonjet sources in Taurus. The empirical relationship discovered by Howard et al. (2013) is shown with a dotted line and provides a useful diagnostic. From its placement among Taurus jet sources, we tentatively identify [OI] emission from J1614-1906 as originating in a jet. Similarly, we identify J1604-2130 as showing emission from a disk.
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