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VLT-ISAAC 3-5 μm spectroscopy of embedded young low-mass stars. III. Intermediate-mass sources in vela

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Figure

Fig. 1. CO (1–0) contour map of the Vela Molecular Cloud complexfilled circles are the location of the 50 other embedded young stellarobjects
Fig. 2. Acquisition image in the stellar field of LLN 17 (IRAS 08448–South and the pixel scale is 14343
Table 1. Characteristics of the sources.
Fig. 3. Optical depth profiles of the 3 µm ice feature for the 5 objects (dotted line) compared to ice coated grains at different radii usinglaboratory spectra taken from (?).
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