Table 1
Regions towards VRO 42.05.01 that show signatures of heating, possibly due to an interaction between the SNR and the molecular cloud.
| Region | RA | Dec | Central velocity (km s−1 ) | FWMH (km s−1) | Ratio | Signal-to-noise ratio of 12CO (J = 1−0) | Signal-to-noise ratio of 12CO (J = 2−1) |
|---|---|---|---|---|---|---|---|
| C | 5:25:53 | +43:07:58 | −5.0 | 2.5 | 1.4 | 5.7 | 6.9 |
| Sw 3 | 5:25:57 | +43:03:39 | −7.0 | ||||
| Sw 1 | 5:25:44 | +43:07:30 | −7.0 | ||||
| A*/Sw 2 | 5:25:41 | +42:48:30 | −7.5 | 13.5 | 2.0 | 9.4 | 9.7 |
| B* | 5:25:20 | +42:45:17 | −10.0 | 11.5 | 1.8 | 7.3 | 8.9 |
| D* | 5:24:57 | +42:56:41 | −14.0 | 10.5 | 1.9 | 4.1 | 4.8 |
| E | 5:25:34 | +43:08:43 | −18.0 | 4.5 | 1.1 | 3.4 | 2.9 |
| G | 5:25:34 | +43:20:59 | −21.5 | 3.0 | 1.5 | 3.0 | 4.0 |
| F | 5:25:29 | +43:17:20 | −22.5 | 2.0 | 1.1 | 6.3 | 5.4 |
| U | 5:25:21 | +43:22:35 | −21.5 | 1.0 | 0.65 | 119.2 | 70.2 |
Notes. Region U is shown as an example of unperturbed emission. The regions indicated with an asterisk show the clearest evidence that the SNR shock is interacting with the molecular gas. The Ratio column shows the ratio of 12CO (J = 2−1) to 12CO (J = 1−0) peaks in the given region. The signal-to-noise ratio columns correspond to the ratio of the peak measured for a given transition to the noise in the empty channels of the same region.
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