Table B.1.
Propynal column densities and upper limits, with associated line parameters.
| Source | Frequency | Transition | Eu | Sijμ2 | Q (Qrot, Qvib) (a) | NT | N(H2) | XH2 | Refs. |
|---|---|---|---|---|---|---|---|---|---|
| (MHz) | ( ) |
(K) | (Debye2) | (cm−2) | (cm−2) | N(H2) | |||
| NGC 6334I | 280106.3 | 304, 26 − 294, 25 | 256.9 | 164.1 | 8323 (6908, 1.20) | ≤3.6 × 1015 | – | – | – |
| Sgr B2(N) | Detection specifics reported in Turner (1991) |  |
1 × 1024 | 4 × 10−11 | 1 | ||||
| Barnard 1 (c) | 102298.1 | 110, 11 − 100, 10 | 29.5 | 61.2 | 142 (142, 1.00) | ≤1.5 × 1011 | 1.5 × 1023 | ≤1 × 10−12 | 3 |
| IRAS 4A | 100716.9 | 111, 11 − 101, 10 | 32.1 | 60.7 | 424 (424, 1.00) | ≤5.6 × 1012 | 3.7 × 1023 | ≤2 × 10−11 | 3 |
| L1157B1 | 85361.2 | 91, 8 − 81, 7 | 23.5 | 49.5 | 2060 (2041, 1.01) | ≤1.1 × 1011 | 1 × 1021 | ≤1 × 10−10 | 3 |
| L1157mm | 104302.2 | 111, 10 − 101, 9 | 33.1 | 60.7 | 2060 (2041, 1.01) | ≤7.0 × 1011 | 6 × 1021 | ≤1 × 10−10 | 3 |
| L1448R2 | 102298.1 | 110, 11 − 100, 10 | 29.5 | 61.2 | 2060 (2041, 1.01) | ≤1.9 × 1012 | 3.5 × 1023 | ≤5 × 10−12 | 4 |
| L1527 | Detected in this work; see text and Table B.2 | 142 (142, 1.00) |  |
2.8 × 1022 | 5 × 10−12 | 4 | |||
| L1544 | 93043.3 | 100, 10 − 90, 9 | 24.6 | 55.7 | 142 (142, 1.00) | ≤6.4 × 1010 | 5 × 1021 | ≤1 × 10−11 | 5 (b) |
| SVS13A | 257153.6 | 280, 28 − 270, 27 | 180.2 | 155.8 | 3255 (3144, 1.04) | ≤2.5 × 1015 | 3 × 1024 | ≤8 × 10−10 | 6 |
| TMC1 | Detection specifics reported in Irvine et al. (1988) |  |
1 × 1022 | 2 × 10−10 | 3 | ||||
Notes.
Calculated at the excitation temperature assumed for the source. See Table A.1.
Jimenez-Serra et al. (2016) reported a column density of (1.8 − 6.3) × 1011 cm−2 based on a single transition.
Loison et al. (2016) reported a detection of propynal in Barnard 1 that is not seen in the ASAI observations with a column density of NT = 7.9 × 1011 cm−2. See text for details.
References.Araki et al. (2017), Lis & Goldsmith (1990); [2] Crockett et al. (2014); [3] Cernicharo et al. (2018); [4] Jørgensen et al. (2002); [5] Vastel et al. (2014); [6] Chen et al. (2009).
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