Table 5
CN outer radii and line detections.
| Source | Radius | T 0 | Line width | Detection? | ||
| (AU) | (K) | km s-1 | 13CO | H2CO | SO | |
|
|
||||||
| FN Tau | <170 | 15 | Cloud | |||
| CW Tau | <170 | 15 | Disk | |||
| CIDA-1 | <170 | 15 | ||||
| BP Tau | <250 | 30 | ||||
| DE Tau | <250 | 15 | ||||
| RY Tau | 310 | 30 | 0.82 ± 0.27 | Disk | ||
| T Tau | 1230 | 30 | 2.96 ± 0.02 | Yes | Yes | |
| Haro 6-5B | 310 | 15 | 3.12 ± 1.17 | Yes | ||
| FT Tau | 310 | 15 | 1.69 ± 0.34 | |||
| DG Tau-B | 450 | 15 | 2.12 ± 0.30 | Yes | Yes | |
| DG Tau | 700 | 30 | 2.11 ± 0.09 | Yes | Yes | |
| Haro 6-10 | 660 | 30 | 1.50 ± 0.04 | Yes | Yes | |
| IQ Tau | 560 | 15 | 4.92 ± 0.53 | Disk | ||
| LkHa 358 | <240 | 15 | Disk | Yes | ||
| HH 30 | <270 | 15 | (Disk) | Yes | ||
| HL Tau | 250 | 30 | 1.79 ± 0.44 | Yes | Yes | |
| HK Tau | 320 | 30 | 8.56 ± 1.96 | |||
| Haro 6-13 |  280 |
15 | Yes | |||
| GG Tau | 490 | 30 | 2.28 ± 0.32 | Disk | Yes | |
| UZ Tau E | 310 | 30 | 6.58 ± 1.23 | Disk | ||
| 04302+2247 | 190 | 30 | 2.99 ± 0.47 | Disk | Yes | Yes |
| DL Tau | 560 | 15 | 1.96 ± 0.16 | Yes | ||
| DM Tau | 610 | 15 | 1.44 ± 0.11 | Disk | Yes | |
| AA Tau | 300 | 15 | 0.95 ± 0.26 | Disk | ||
| DN Tau | 490 | 15 | 3.21 ± 0.42 | Yes | ||
| DO Tau | 310 | 15 | 0.50 ± 0.17 | Disk | Yes | |
| HV Tau C | 310 | 30 | 5.97 ± 0.87 | Disk | ||
| Haro 6-33 | 260 | 30 | 3.05 ± 0.68 | Yes | ||
| DQ Tau | <210 | 15 | ||||
| DR Tau | <420 | 15 | ||||
| DS Tau | <310 | 30 | Yes | |||
| UY Aur | <300 | 30 | Disk | Yes | ||
| AB Aur | <250 | 30 | Disk | Yes | ||
| SU Aur | <140 | 30 | Disk | |||
| MWC 480 | 520 | 30 | 4.54 ± 0.34 | Disk | ||
| CB 26 | 350 | 15 | 2.92 ± 1.00 | Yes | Yes | |
| CIDA-8 | <290 | 15 | Cloud | |||
| CIDA-11 | <540 | 15 | ||||
| RW Aur | <280 | 30 | ||||
| MWC 758 | <450 | 30 | Disk | |||
| CQ Tau | <190 | 30 | Disk | Yes | ||
| HD 163296a | 760 | 30 | 4.16 ± 0.11 | Disk | Yes | |
Notes. The assumed distance is D = 140 pc, except for HD 163296 (a, D = 120 pc). For 13CO, sources in which the emission partially originates from a disk are indicated. For H2CO, no distinction is made upon the origin of the emission, apart from the two likely cases of cloud confusion FN Tau and CIDA-8.
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