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. Author manuscript; available in PMC: 2018 Aug 1.
Published in final edited form as: Astrophys J Suppl Ser. 2017 Aug 18;231(2):22. doi: 10.3847/1538-4365/aa8175

Table 10.

Comparison of Each of the Mass Components between This Work and the HerPlaNS1 Results

Parameters This Work HerPlaNS1 HerPlaNS1 (Scaled)
D (kpc) 0.46 0.95 0.46
Filling factor 1.0 0.5 1.0
Total gas (M) 0.41 0.86 0.40
Ionized gas (M) 0.09 0.54 0.25
Atomic gas (M) 0.20 0.12 0.05
Total molecular gas (M) 0.11 0.20 0.09
Warm molecular gas (M) 4.15(−3)
Cold molecular gas (M)a 1.12(−1)
Total dust mass (M) 1.53(−3)
Dust mass beyond RIB (M) 1.06(−3) 4.0(−3)b 9.4(−4)b
GDR 268 335 (median) 335 (median)

Notes.

a

The model-predicted cold molecular mass was scaled from the model-predicted warm molecular mass in this work. In HerPlaNS1, the molecular component was not subdivided by temperature.

b

The empirical dust mass estimate was for the cold dust of 20–40 K.