Table B.2.
Literature comparison of J = 2−1 12CO/13CO
| NGC | This | Lit. | Ratio | Telescope (a) | Ref |
|---|---|---|---|---|---|
| paper | value | ||||
| (1) | (2) | (3) | 4) | (5) | (6) |
| 660 | 17.0 | 21.8 | 0.78 | O | 6,10 |
| 1068 | 12.8 | 10 | 1.28 | J | 1 |
| 1365 | 11.5 | 10/13 | 0.98 | J/SMA | 5/22 |
| 1808 | 12.6 | 15.5 | 0.81 | S | 6,10 |
| 2146 | 8.7 | 9.9 | 0.88 | O | 6,10 |
| 3034 | 10.8 | 11.9 | 0.91 | J | 24 |
| 3034 | 14.3 | 11.3 | 1.29 | I | 25 |
| 3227 | 13.5 | 25 | 0.54 | J | 5 |
| 3256 | 16 | 10/21/23/17 | 0.90 | S/SMA | 6,10,8/27 |
| 4039 | 12.9 | 12.0 | 13/13/10 | C/J/I | 3/15/16 |
| 4038 | 15.8 | 19.8 | 27/16/16 | C/J/I | 3/15/16 |
| 4051 | 21 | 14 | 1.50 | J | 5 |
| 4414 | 8.5 | 9 | 0.94 | I | 18 |
| 4736 | 10.1 | 13.6 | 0.74 | C | 3 |
| 4826 | 5.1 | 5.3 | 0.96 | O | 6,10 |
| 5033 | 8.3 | 6 | 1.38 | J | 5 |
| 5135 | 9.1 | 13 | 0.70 | J | 5 |
| 6240 | 40 | 53 | 0.75 | J | 1 |
| 6764 | 24 | 15 | 1.60 | I | 20 |
| 7331 | 6.2 | 6 | 1.03 | I | 29 |
| 7469 | 17 | 15 | 1.13 | J | 5 |
Notes.
S: Swedish-ESO Submillimeter Telescope (SEST); O: Onsala Space Observatory (OSO); I: Institut Radio Astronomie Millimétrique – Pico Veleta (IRAM); J: James Clerk Maxwell Telescope (JCMT); C: Caltech Submillimeter Telescope (CSO) SMA: Smithsonian Millimeter Array.
References to Tables B.1 and B.2. (1) Papadopoulos et al. (2012); (2) Tan et al. (2011); (3) Glenn & Hunter (2001); (4) Paglione et al. (2001); (5) Papadopoulos & Seaquist (1998); (6) Aalto et al. (1995); (7) Garay et al. (1993); (8) Casoli et al. (1992); (10) Aalto et al. (1991a,b); (11) Young & Sanders (1986); (12) Rickard & Blitz (1985); (13) Encrenaz et al. (1979); (15) Zhu et al. (2003); (16) Schulz et al. (2007); (18) Braine et al. (1993b); (19) Golla & Wielebinsky (1994) (20) Eckart et al. (1991); (21) Sakamoto et al. (1997); (22) Sakamoto et al. (2007); (23) Sandqvist et al. (1988); (24) Petitpas & Wilson (2000); (25) Mao et al. (2000); (26) Costagliola et al. (2011); (27) Sakamoto et al. (2014); (28) Vila-Vilaro et al. (2015); (29) Krips et al. (2010); (30) Muraoka et al. (2016); (31) Cormier et al. (2018).
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