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The physical and chemical evolution of star forming regions

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Figure

Table 1.1: Table of observed interstellar and circumstellar molecules. We also de­note the wavelength ranges of the detections if they are not made at millimetre wavelengths
Table 1.3: Some important timescales. From Hartquist k  Williams 1998.
Figure 1.2: The distribution of dark cores and low-mass stars in the Taurus — Auriga
Figure 1.3:
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