Table 3.
N-ethylformamide column densities.
Orion KL (c) | Sgr B2 (d) | |
---|---|---|
(ALMA SV) | (IRAM 30 m) | |
Coordinates | α = 5h35m14.5s | α = 17h47m20.0s |
(J2000.0) | δ = −05°22′33.0″ | δ = −28°22′19.0″ |
HPBW (a) (″) | ∼2.0 × 1.5 | 30–21 |
Frequency (b) (GHz) | 213.7–246.6 | 80–115.5 |
vLSR (km s−1) | 8.0 | 63.0 |
ΔvFWHM (km s−1) | 3.0 | 7.0 |
dsou (″) | 3.0 | 2.4 |
Trot (K) | 150 | 180 |
N(NH2CHO) (cm−2) | 3.0 × 1015 | 1.3 × 1018 |
N(CH3NHCHO) (cm−2) | ≤1.0 × 1015 | ≤2.0 × 1017 |
N(NEFA) (cm−2) | ≤1.0 × 1014 | ≤1.0 × 1017 |
N(NH2CHO)/N(CH3NHCHO) | ≥3 | ≥6.5 |
N(NH2CHO)/N(NEFA) | ≥30 | ≥13 |
Notes.
HPBW (half power beam width) for observations with single-dish telescope (IRAM 30m) and synthetic beam for the ALMA SV observations.
Physical parameters derived for the main spectral component of NH2CHO by Cernicharo et al. (2016).
Physical parameters derived for the main spectral component of NH2CHO by Belloche et al. (2013).
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