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Table 3

Synopsis of derived quantities.

Source υLSR Range RGAL (a) N(ArH +) N(OH +) N(p -H2O +) N(o-H2O+) H2O+ N(HI) ζp(H)

(km s−1) (kpc) (1012 cm−2) (1014 cm−2) (1013 cm−2) (1013 cm−2) OPR (1021 cm−2) OH+ (b) CH(c) (10−16 s−1)
AG10.472 (− 35, 0) 10.82 <0.019 <4.52
+00.027 (0, 48) 5.56 >1.05 <3.26 >0.031 >4.52
(48, 77)(d) 3.50 >0.005 >2.48
(77, 105) 3.12
(105, 138) 2.38
(138, 190) 1.48
AG19.609 (− 12, 16) 8.04
−00.234 (16, 35) 6.75
(35, 60)(d) 4.50
(60, 87) 4.34
(87, 105) 3.32
(105, 115) 3.01
(115, 135) 2.73
AG31.412 (− 8, 31)(*) 7.05
+00.307 (31, 46)(*) 6.39 <0.05
(46, 65)(*) 5.49 >0.08 <1.13
(65, 88)(*) 4.71
(88, 108)(d,*) 4.64 >0.776 >1.08
AG330.954 (− 130, −74)(d) 4.43 >1.24
−00.182 (− 74, −57) 4.92 >0.026 >1.62
(− 57, −32) 5.78
(− 32, −10) 7.03
(− 10, 20) 8.54 >0.058
AG332.826 (− 85, −33)(d) 5.30
−00.549 (− 33, −12) 7.02 >0.24 >2.04
(− 12, 20) 8.67
AG337.704 (− 145, −110) 3.12
−00.054 (− 110, −97) 3.25
(− 97, −80) 3.73 (e)
(− 80, −65) 4.43
(− 65, −45)(d) 5.17
(− 45, −25) 5.29
(− 25, −13) 6.91 >0.048
(− 13, 7) 8.62 >0.026
AG351.581 (− 120, −70)(d) 1.66
−00.352 (− 70, −39) 3.18 >0.554
(− 39, −7) 4.50
(− 7, 25) 9.74

Notes. (a) The galactocentric distance for each velocity interval is computed using, RGAL = , with R0 = 8.15 kpc, Θ0 = 247 km s−1 (Reid et al. 2019) and assuming a flat Galactic rotation curve, i.e., Θ(RGAL) = Θ0 for RGAL > 5 kpc. We used the BeSSeL distance calculator, to both cross-check and determine lower RGAL values. The distances are computed at the mean velocity within each velocity interval. (b,c) Represent values derived using Eqs. (4) and (3), respectively. Where H2 column densities for the latter are determined from those of CH (Jacob et al. 2019) using [CH]/[H2] = (Sheffer et al. 2008). (d)Indicates the velocity intervals corresponding to the molecular cloud. (e) Faces a singularity as the denominatorapproaches 0. (*)Represents velocity intervals with low signal-to-noise ratios, for which molecular hydrogen fractions are calculated using the upper limits of the derived N(OH+) values.

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