Fig. 3
Characteristic line profiles observed with the IRAM 30 m telescope in the λ3 mm band toward L483. Left panel: lines with wings and self-absorption (except C18O J = (1–0)). Middle panel: lines that show wings. Right panel: sample of narrow lines, which form the majority in our line survey. The gray shaded area indicates the velocity range ± 0.5 km s−1 around the systemic velocity of the source.
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