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The environments in which stars and circumstellar discs form

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Figure

Table 1.1: Stellar and disc parameters of the stars imaged at submillimetre wave- wave-lengths.
Figure 1.2: Theoretical evolutionary Hayashi-Henyey tracks for stars of various masses between 0.05-4 M ¯ under going quasi-hydrostatic collapse
Figure 1.3: Schematic of SED models associated with Class 1 (Envelope), Class II (Disc) and Class III (Remnant Disc) objects
Figure 2.2: A diagram demonstrating how a radiation hit (right) is distinguished from a bright point source (left) and a faint point source (centre)
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