Table 2.
Estimates of the CO-to-H2 conversion factors, gas masses and gas-to-dust ratios.
Source | αCO | μMCO(H2) | MCO(H2) | ![]() |
![]() |
δGDR |
---|---|---|---|---|---|---|
(M⊙ (K km s−1 pc2)−1) | (1011 M⊙) | (1010 M⊙) | (1011 M⊙) | (1011 M⊙) | ||
PLCK_G045.1+61.1 | 0.78 ± 0.30 | 8.6 ± 0.4 | 5.5 ± 0.5 | 4.3 ± 1.2 | 3.9 ± 1.2 | 220 ± 18 |
PLCK_G080.2+49.8 | 1.82 ± 0.46 | 1.0 ± 0.1 | 0.6 ± 0.1 | ... | ... | 22 ± 5 |
PLCK_G092.5+42.9 | 0.90 ± 0.40 | 8.3 ± 0.4 | 6.9 ± 0.7 | 7.5 ± 1.4 | 5.7 ± 1.5 | 273 ± 34 |
PLCK_G102.1+53.6 | ... | 1.6 ± 0.2 | 2.3 ± 0.4 | ... | ... | 84 ± 13 |
PLCK_G113.7+61.0 | 1.03 ± 0.41 | 5.8 ± 0.2 | 6.0 ± 0.5 | ... | ... | 262 ± 30 |
PLCK_G138.6+62.0 | 0.85 ± 0.35 | 4.5 ± 0.2 | 2.2 ± 0.7 | ... | ... | 15 ± 8 |
PLCK_G145.2+50.9 | 1.02 ± 0.41 | 10.5 ± 0.4 | 11.8 ± 1.1 | ... | ... | 111 ± 9 |
PLCK_G165.7+67.0 | 0.73 ± 0.26 | 8.1 ± 0.2 | 3.4 ± 0.8 | ... | ... | 265 ± 68 |
PLCK_G200.6+46.1 | ... | 4.2 ± 0.3 | 2.8 ± 1.0 | ... | ... | 133 ± 74 |
PLCK_G231.3+72.2 | ... | 2.5 ± 0.3 | 4.2 ± 0.9 | ... | ... | 96 ± 16 |
PLCK_G244.8+54.9 | ... | 5.7 ± 0.3 | 2.6 ± 0.3 | 3.4 ± 1.1 | 3.0 ± 1.0 | 203 ± 19 |
Notes. The αCO column lists the CO luminosity to gas mass conversion factors, expressed in units of M⊙ (K km s−1 pc2)−1 and deduced from the [C I]-inferred molecular gas masses for the sources with [C I](1–0) detections (Nesvadba et al. 2018, see further details in the text). The molecular hydrogen masses, μMCO(H2), are derived from the modeled CO(1–0) luminosities assuming αCO = 0.8 M⊙ (K km s−1 pc2)−1. Intrinsic values are corrected for the magnification factors μgas of Table 1. We also list the gas masses inferred for the individual kinematic components in three Planck’s dusty GEMS. The quantities δGDR are the gas-to-dust mass ratios deduced from the dust masses presented in C15, corrected for μdust, and the total molecular gas masses, MCO(H2). Errors include uncertainties on the line fluxes and magnification factors.
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