All Figures

$\begin{figure} \par\includegraphics[angle=0,width=8cm,clip]{fig1CMJN.eps} \end{figure}$ Figure 1: Dust continuum mosaic (contours and grey scale) of the Serpens main core as observed with the IRAM 30 m telescope. The location of the Class II (blue filled squares), flat (red crosses) and Class I sources (red empty circles) is indicated (adapted from Kaas et al. 2004). In the inset, we show the 3 mm and 1.3 mm (small inset) continuum images observed with the PdBI. Note that only one compact core is detected in this region down to a spatial scale of less than 100 AU. The dashed circle marks a region of 0.2 pc radius around FIRS 1.
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In the text

$\begin{figure} \par\includegraphics[angle=0,width=17cm,clip]{fig2CMJN.eps} \end{figure}$ Figure 2: On the left, we show the 5 $'\times 5'$ Spitzer IRAC 3.6 $\mu$ m image towards IC 1396 N (adapted from Getman et al. 2007). The location of the globule is marked by the green contour and the Class III (yellow triangles), Class II (red circles) and blue squares (Class 0/I) sources are indicated. On the right, we show the 3 mm (up) and 1.3 mm (down) continuum images observed with the PdBI. In the 3 mm image we also indicate the Class III (black triangles), Class II (red circles) and Class 0/I (filled blue squares) sources.
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In the text

$\begin{figure} \par\includegraphics[angle=0,width=8.2cm,clip]{fig3CMJN.eps} \end{figure}$ Figure 3: Dust continuum emission at 850 $\mu$ m as observed with SCUBA towards CB 3. In the inset, we show the 3 mm continuum image observed with PdBI. Note that two compact cores are detected towards the single-dish peak.
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In the text

$\begin{figure} \par\includegraphics[angle=0,width=8.2cm,clip]{fig3CMJN.eps} \end{figure}$	Figure 3: Dust continuum emission at 850 $\mu$ m as observed with SCUBA towards CB 3. In the inset, we show the 3 mm continuum image observed with PdBI. Note that two compact cores are detected towards the single-dish peak.
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