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Table 1.

Properties of the molecular lines and images analysed in this work.

Molecule Transition Frequency log10(Aij) Eup gu Beam Δv Peak rms (*) Disk int. flux
(GHz) (s−1) (K) kms−1 (mJy beam−1) (mJy km s−1)
C18O 3–2 329.3305525 −5.6631 31.6 7 020 × 016 (65°) 0.23 58.45 5.10 896.5 ± 90
SO2 53, 3–42, 2 351.2572233 −3.0672 35.9 11 055 × 044 (80°) 1.7 34.33 0.91 305.1 ± 31
SO2 144, 10–143, 11 351.8738732 −3.4644 135.9 29 055 × 044 (80°) 1.7 13.87 0.91 124.9 ± 12
34SO2 63, 3–52, 4 362.1582327 −3.4839 40.7 13 053 × 042 (80°) 1.7 12.11 1.20 87.3 ± 9
SO 12–01 329.3854770 −4.8467 15.8 3 020×016 (65°) 1.7 (**) 13.62 2.49 166.9 ± 17
CS 7–6 342.8828503 −3.0774 65.8 15 020×016 (65°) 0.23 – 8.23 < 348 ± 35

Notes. (*)Per channel. (**)The native channel width of these data is 0.23 km s−1. The values for the line frequencies, Einstein A coefficients, and upper energy levels (Eup) and degeneracies (gu) are taken from the Cologne Database for Molecular Spectroscopy (CDMS; Müller et al. 2005).

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