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	Figure 1: Mid-infrared images of GGD 14 (IRAS 06084-0611). For comparison, the 2.2  image by Kodapp (1994) is also shown at the same scale. The positions of the continuum radio sources found by Gómez et al. (2002), are marked on the 12.5  image. North is the top and east to the left.
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In the text

	Figure 2: The PHT-S spectrum towards the IRAS source 06084-0611. The open circles represents our observed flux densities of the source VLA 4 (Irs2). The bars show the widths of the mid-infrared filters.
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In the text

	Figure 3: Contour maps at 12.5  (left panel) and at 3.6 cm (right panel) from (Gómez et al. 2002) of the star forming region GGD 14 around IRAS 06084-0611. The contour levels in the 12.5  map are: 0.36, 0.45, 0.54, 0.62, 0.71, 0.80 and 0.89 Jy/arcsec2.
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In the text

	Figure 4: J-Hvs. H-K diagram of the VLA sources in the GGD 14 region. The continuous line marks the locus of the main sequence stars from Koornneef (1983). The two parallel lines represent the standard reddening vectors for late and early-type stars.
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In the text

	Figure 5: Spectral energy distribution of VLA 1. The symbols are: open circles from Harvey et al. (1985), open squares from Little et al. (1990) with a 15 beam, filled circles from this work. The K upper limit is taken from 2MASS.
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In the text

	Figure 6: Left panel: SED of VLA 4. The symbols are: open circles from Harvey et al. (1985) and filled circles from this work. Right panel: SED of VLA 2. The symbols are: open circles from Harvey et al. (1985) and filled squared from 2MASS.
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In the text