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Table 4

Peak abundances and abundance ratios for NO-related species obtained from our model and a comparison of peak abundance ratios with the available observation.

Species Dark cloud Hot core Observation
HONO 7.7 × 10−13(g)/2.3 × 10−9(s) 1.5 × 10−11(g)/3.8 × 10−8(s)
NO 8.6 × 10−8(g)/8.6 × 10−8(s) 3.2 × 10−7g/3.2 × 10−8(s)
N2O 4.2 × 10−9(g)/4.7 × 10−9(s) 4.4 × 10−6(g)/8.3 × 10−8(s)
HNO 5.8 × 10−9(g)/5.6 × 10−9(s) 1.5 × 10−10(g)/7.1 × 10−12(s)
NO2 1.2 × 10−10(g)/3.8 × 10−10(s) 2.5 × 10−13(g)/2.3 × 10−13(s)
NH2OH 3.6 × 10−12(g)/2.2 × 10−14(s) 5.0 × 10−6(g)/2.1 × 10−10(s)
CH3OH 9.2 × 10−9(g)/9.2 × 10−9(s) 3.1 × 10−5(g)/3.3 × 10−5(s)
HONO/NO 8.9 × 10−6(g)/0.03(s) 4.7 × 10−5(g)/1.2(s) 4.5 × 10−2(c)
HONO/N2O 0.0002(g)/0.5(s) 3.4 × 10−6(g)/0.4(s) ≤2.3 × 10−2(c)
HONO/HNO 0.0001(g)/0.4(s) 0.08(g)/3781(s) ≥3(c)
HONO/NO2 0.006(g)/6.1(s) 56(g)/9.8 × 104(s) ≥4.5 × 10−2(c)
HONO/NH2OH 0.22(g)/1.0 × 105(s) 2.9 × 10−6(g)/143(s) ≥2.3(c)
HONO/CH3OH 8.4 × 10−5g/0.25(s) 4.8 × 10−7(g)/0.001(s) 9 × 10−5(c)

Notes. (c)Coutens et al. (2019) in the low−mass protostellar source IRAS 16293–2422 B.(g) When the BEs from Garrod (2013) are used.(s) When the BEs calculated here are used (otherwise those from Garrod 2013 are used).

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