Table A.1.
Data of JFCs, HFCs, OCCs, and Centaurs for which we both have measurements of QCO and diameter. QCO is the CO production rate in s−1, and its error bar is the 1σ uncertainty. D is the equivalent nucleus diameter in km, and rh is the heliocentric distance of the object in au. The upper limits are represented by the 3σ uncertainties.
| Name | QCO | D | rh | ref |
|---|---|---|---|---|
| C/1995O1 | 6.5 ± 0.8 × 1027 | 69.9 | 14.07 | (1) |
| C/1995O1 | 2.15 ± 0.17 × 1030 | 69.9 | 0.917 | (1) |
| C/1996B2 | 1.2 ± 0.3 × 1028 | 2.29 | 1.852 | (2) |
| C/1996B2 | 10.4 ± 2.4 × 1028 | 2.29 | 0.478 | (2) |
| C/2020F3 | 1.3 ± 0.5 × 1028 | 5.0 | 0.71 | (3) |
| 10199 | < 15.0 × 1027 | 249 | 13.5 | (4,5) |
| 1P | 4.5 ± 2 × 1028 | 9.3 | 0.92 | (6) |
| 2P | 1.8 ± 0.2 × 1026 | 7.02 | 0.473 | (7) |
| 8P | 2.4 ± 0.4 × 1026 | 4.93 | 1.027 | (8) |
| 9P | 8.7 ± 1.6 × 1026 | 6.07 | 1.506 | (8) |
| 10P | < 7.8 × 1027 | 9.24 | 1.482 | (9) |
| 19P | < 4.5 × 1027 | 4.34 | 1.360 | (10) |
| 21P | 4.6 ± 0.8 × 1026 | 3.6 | 1.18 | (11) |
| 21P | 2.5 ± 0.3 × 1026 | 3.6 | 1.10 | (11) |
| 22P | < 8.1 × 1025 | 3.77 | 1.61 | (12) |
| 29P | 3.5 ± 1.5 × 1028 | 56.3 | 6.0 | (13,14) |
| 41P | < 8.4 × 1026 | 1.4 | 1.06 | (15) |
| 45P | 1.9 ± 0.3 × 1026 | 0.92 | 0.555 | (16) |
| 46P | < 3.3 × 1025 | 1.2 | 1.13 | (17) |
| 67P | 3.4 ± 2.5 × 1026 | 3.81 | 1.28 | (18,19) |
| 73PC | 7 ± 2 × 1025 | 1.61 | 0.950 | (8) |
| 81P | > 5.3 × 1025 | 4.17 | 1.74 | (12) |
| 95P | 1.3 ± 0.6 × 1028 | 155 | 8.5 | (20,21) |
| 95P | < 8.1 × 1027 | 155 | 8.48 | (22,21) |
| 95P | < 5.1 × 1028 | 155 | 8.9 | (4,21) |
| 103P | 2.6 ± 0.3 × 1025 | 0.68 | 1.064 | (23) |
| 174P | 8.0 ± 3.0 × 1026 | 64 | 6.13 | (14) |
References. (1): Biver et al. (2002); (2): Biver et al. (1999); (3): Biver et al. (in prep.); (4): Bockelée-Morvan et al. (2001); (5): Morgado et al. (2021); (6): Feldman et al. (1997); (7): Roth et al. (2018); (8): Dello Russo et al. (2016), and references therein); (9): Biver et al. (2012); (10): Bockelée-Morvan et al. (2004a); (11): Roth et al. (2020); (12): Ootsubo et al. (2012); (13): Crovisier et al. (1995); (14): Wierzchos et al. (2017); (15): Biver et al. (2021); (16): DiSanti et al. (2017); (17): McKay et al. (2021); (18): Biver et al. (2019); (19): Läuter et al. (2020); (20): Womack et al. (2017); (21): Lellouch et al. (2017); (22): Rauer et al. (1997); (23): Weaver et al. (2011).
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