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Table A.3.
13CO J = 1–0 observations in our sample.
| Source | 1σ noise | A | Tmb | FWHP |
|---|---|---|---|---|
| (K) | (K km s−1) | (K) | (km s−1) | |
| VX And | 0.007 | < 0.54 | < 0.02 | – |
| V370 And | 0.011 | 1.25 | 0.15 | 4.94 |
| Z Eri | 0.008 | < 0.37 | < 0.02 | – |
| SS Cep | 0.009 | 0.24 | 0.04 | 12.71 |
| TT Tau | 0.008 | 0.13 | 0.02 | 10.77 |
| W Ori | 0.013 | < 0.94 | < 0.04 | – |
| RX Lep | 0.012 | < 0.41 | < 0.04 | – |
| Y Tau | 0.011 | 0.29 | 0.04 | 30.72 |
| S Lep | 0.006 | < 0.37 | < 0.02 | – |
| RY Mon | 0.009 | < 0.66 | < 0.03 | – |
| RT Hya | 0.009 | < 0.21 | < 0.03 | – |
| RT Cnc | 0.009 | < 0.47 | < 0.03 | – |
| R Crt | 0.017 | 1.03 | 0.09 | 19.95 |
| Z UMa | 0.008 | < 0.17 | < 0.02 | – |
| BK Vir | 0.009 | 0.11 | 0.04 | 7.24 |
| Y UMa | 0.011 | 0.39 | 0.07 | 7.24 |
| Y CVn | 0.014 | 6.71 | 0.47 | 15.36 |
| RT Vir | 0.013 | 0.82 | 0.08 | 12.36 |
| SW Vir | 0.015 | 0.63 | 0.07 | 13.60 |
| RX Boo | 0.013 | 1.00 | 0.10 | 16.07 |
| τ4 Ser | 0.007 | < 0.73 | < 0.02 | – |
| ST Her | 0.010 | < 0.75 | < 0.03 | – |
| X Her | 0.014 | 1.30 | 0.14 | 5.65 |
| g Her | 0.008 | 0.42 | 0.04 | 12.89 |
| S Dra | 0.010 | 0.27 | 0.03 | 9.00 |
| FI Lyr | 0.008 | 0.24 | 0.03 | 8.65 |
| S Sct | 0.016 | 0.08 | 0.02 | 5.70 |
| AF Cyg | 0.010 | 0.20 | 0.04 | 5.83 |
| AQ Sgr | 0.008 | 0.12 | 0.02 | 17.65 |
| RT Cap | 0.008 | 0.06 | 0.02 | 3.00 |
| UU Dra | 0.009 | 0.63 | 0.07 | 12.54 |
| EU Del | 0.009 | 0.22 | 0.02 | 17.30 |
| U Del | 0.010 | 0.33 | 0.03 | 18.72 |
| IQ Aqr | 0.007 | < 0.54 | < 0.02 | – |
| W Cyg | 0.009 | 0.40 | 0.04 | 15.36 |
| RU Cyg | 0.005 | 0.10 | 0.02 | 15.89 |
| EP Aqr | 0.015 | 2.20 | 0.28 | 2.65 |
| TW Peg | 0.010 | 0.40 | 0.06 | 15.36 |
| SV Lyn | 0.010 | 0.35 | 0.11 | 3.18 |
| SV Peg | 0.013 | 0.63 | 0.08 | 14.05 |
| AK Hya | 0.015 | 0.31 | 0.05 | 9.00 |
| RW Boo | 0.006 | 0.05 | 0.02 | – |
| IQ Her | 0.009 | 0.24 | 0.06 | 6.35 |
| AA Cyg | 0.012 | 0.15 | 0.04 | 4.07 |
| X Cnc | 0.012 | < 0.59 | < 0.04 | – |
| V465 Cas | 0.006 | < 0.39 | < 0.02 | – |
Notes. Description of the columns from left to right: (1) GCVS designation (Samus et al. 2009); (2–5) 1σ noise, integrated line intensity, peak main-beam brightness temperature, and full width at half power. 3σ upper detection limits are indicated.
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