Table 3
Transition properties of lines analyzed in this work.
Line | v0 (GHz) | log Aul (log s−1) | Eu/kB (K) | SPR spw |
---|---|---|---|---|
H(40)α | 99.023 | … | … | SPR2 spw6 |
HCN 1−0 | 88.630 | −4.6 | 4 | SPR1 spw5 |
HNC 1−0 | 90.664 | −4.6 | 4 | SPR3 spw9 |
CH3CN 54−44 | 91.959 | −4.8 | 128 | SPR3 spw13 |
CH3CN 53−43 | 91.971 | −4.6 | 78 | SPR3 spw13 |
CH3CN 52−42 | 91.980 | −4.4 | 42 | SPR3 spw13 |
CH3CN 51−41 | 91.985 | −4.4 | 20 | SPR3 spw13 |
CH3CN 50−40 | 91.987 | −4.4 | 13 | SPR3 spw13 |
![]() |
91.913 | −4.6 | 128 | SPR3 spw11 |
![]() |
91.926 | −4.4 | 78 | SPR3 spw11 |
![]() |
91.935 | −4.3 | 42 | SPR3 spw11 |
![]() |
91.940 | −4.2 | 20 | SPR3 spw11 |
![]() |
91.942 | −4.2 | 13 | SPR3 spw11 |
Notes. The line properties are taken from the Cologne Database for Molecular Spectroscopy (CDMS, Müller et al. 2005) and the Jet Propulsion Laboratory (JPL; Pickett et al. 1998) database. The last column refers to the corresponding line data product (SPR and spw) that covers the transition in the ALMA observations (Table A.2).
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