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Weak and compact radio emission in early high mass star forming regions II The nature of the radio sources

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Figure

Figure 1. The distance distribution of our targets is shown as a black line. The color histogram shows the number of targets where we expect the detection of T-Tauristars which are as bright as J162749.85–242540.5 in Ophiuchus
Table 1
Figure 3. Initial Strömgren sphere radius as a function of the Lymanconstant density Hrepresent the radius of the Hareas represent the path from their initial radius up to theirsphere radius if the sources were born at a density ofrespectively20% calibrati
Figure 4produced by higher free, we also show several UC H II regions from Kurtz et al.(1994), denoted by the × symbol
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