Table 4
Sizes measured at noise level in the 30 m telescope maps.
| Source | 12CO J = 1−0 | 12CO J = 2−1 | Photodiss. |
| CSE size | CSE size | diameter | |
|
|
|||
| TX Cam | 77″ | 69″ | 52″ |
| V Cyg | ≳ 90″* | 48″ | 39″ |
| χ Cyg | 97″ | 81″ | 76″ |
| RX Boo | 75″ | 52″ | 62″ |
| S Cep | 78″ | 48″ | 28″ |
| R Cas | 85″ | 65″ | 53″ |
Notes. The shown angular sizes are not corrected from the contribution of the 30 m telescope primary beam. Theoretical estimates of the photodissociation diameter are also given.(*) The measured size is apparently larger than the observed field, of ~100″, perhaps due to ISM contamination at the systemic velocity. For TX Cam and V Cyg the envelopes look slightly elongated, with a size difference of ~4−8″; the mean angular size is given in the table.
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