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Table 3
HC3N 24−23 spectral measurements.
| Source | On-time | RMS | δV | ΔV | V 0 | I(HC3N) | S(HC3N) |
|
| (min) | (mK) | (km s-1) | (km s-1) | (km s-1) | (K km s-1) | (Jy km s-1) | ||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) |
|
|
||||||||
| NGC 1068 | 121 | 1.2 | 39.1 | 257.3 (24.0)a | 1102 (13) | 2.03 (0.18) | 49.9 (4.4) | ~0.59 |
| IC 342 | 132 | 2.7 | 20.9 | 100b | 43 | 0.47 (0.12) | 11.6 (3.0) | ~0.12 |
| IC 694 | 127 | 0.87 | 41.7 | 400b | 3095 | 0.90 (0.11) | 22.1 (2.7) | ~2.76 |
| NGC 2146 | 115 | 1.01 | 20.9 | 320c | ... | <0.17 | 4.2 | <0.26 |
| M 82 | 60 | 3.0 | 20.9 | 150c | ... | <0.34 | 8.4 | <0.26 |
| NGC 3690 | 139 | 0.73 | 42.0 | 260c | ... | <0.15 | 3.7 | <1.27 |
| ARP 220 | 162 | 0.75 | 39.1 | 420c | ... | <0.19 | 4.7 | <0.48 |
| NGC 6240 | 97 | 0.92 | 20.1 | 420c | ... | <0.17 | 4.2 | <1.15 |
| NGC 6946 | 168 | 1.76 | 21.0 | 130c | ... | <0.18 | 4.4 | <0.26 |
Notes.Columns are the same as Table 2.
(c)
CO width from Young et al. (1995) that are used to derived the upper limits.
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