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Modélisation 3D de régions de formation d'étoiles. La contribution de l'interface graphique GASS aux codes de transfert radiatif

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Figure

Fig. 1.3 shows the classification of proto-stars as a function of the spectral energy distribution of the dust continuum emission (Adams et al., 1987; Andre et al., 1993; Andre and Montmerle, 1994; Andre, 1994).
Figure 1.6 – Representation of the different movements a molecule can adopt. Taken from Principles
Figure 1.8 – Spectrum of the first 46 rotational transitions of HCO + . The intensities of the
Figure 1.12 – Sketch showing the different components of the antenna of a single-dish telescope and its data processing pipeline.
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