Table 2
Molecular lines and frequencies.
Molecule | J + 1 → J | Eu/kB | Frequency | n crit a | Bandwidth | Resolution | Beam | B eff | F eff | 1σ rms |
(K) | (GHz) | (cm-3) | (MHz) | (km s-1) | (′′) | (K) | ||||
| ||||||||||
IRAM 30 m telescope | ||||||||||
H13CO+ | 1–0 | 4.16 | 86.754 | 1.7 × 105 | 160 | 0.16 | 29 | 0.78 | 0.98 | 0.06 |
SiO | 2–1 | 6.25 | 86.847 | 7.3 × 105 | 160 | 0.16 | 29 | 0.78 | 0.98 | 0.07 |
HCO+ | 1–0 | 4.28 | 89.189 | 1.8 × 105 | 40 | 0.08 | 28 | 0.78 | 0.98 | 0.10 |
CH3CN | 5–4, K = 0, 1, 2, 3, 4 | 13.24b | 91.987b | 4.7 × 105 | 120 | 0.16 | 27 | 0.78 | 0.98 | 0.09 |
N2H+ | 1–0 | 4.47 | 93.174 | 1.6 × 105 | 40 | 0.08 | 27 | 0.78 | 0.98 | 0.11 |
C18O | 2–1 | 15.81 | 219.560 | 9.2 × 103 | 512 | 1.5 | 12 | 0.62 | 0.94 | 0.12 |
CO | 2–1 | 16.60 | 230.538 | 1.1 × 104 | 512 | 1.5 | 11 | 0.58 | 0.92 | 1.3 |
APEX telescope | ||||||||||
N2H+ | 3–2 | 26.83 | 279.512 | 3.0 × 106 | 1000 | 0.15 | 22 | 0.73 | 0.97 | 0.23 |
H2CO | 404–303c | 34.90 | 290.623 | 9.2 × 106 | 1000 | 0.15 | 22 | 0.73 | 0.97 | 0.20 |
HCO+ | 4–3 | 42.80 | 356.734 | 9.1 × 106 | 1000 | 0.12 | 18 | 0.73 | 0.97 | 0.47 |
CO | 3–2 | 33.19 | 345.796 | 3.5 × 104 | 1000 | 0.12 | 18 | 0.73 | 0.97 | 1.1 |
Notes. Columns are (from left to right) the molecule, its transition, its upper energy level, its frequency, its critical column density, the bandwidth used in the observation, the velocity resolution of the observation, the telescope beam, the main beam and forward beam efficiency of the observation, and the mean 1σ noise value. .
Calculated from the collision rates at T = 20 K from the LAMBDA molecular database (Schöier et al. 2005).
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