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. Author manuscript; available in PMC: 2016 Jun 6.
Published in final edited form as: Astrophys J. 2016 May 20;823(1):25. doi: 10.3847/0004-637X/823/1/25

Table 3.

Calculated abundances of CH3O relative to methanol at 10 K considering gas-phase formation via reaction (1)

Grain surface source of CH3O nH
(molecule cm−3
k1(10 K)
(cm3 molecule−1 s−1)
n(CH3O)/n(CH3OH) time (yr) Reference
NO 2 × 104 1.1 × 10−10 (0.08 – 2) × 10−3 105 – 107 This work
NO 1 × 105 1.1 × 10−10 (0.1 – 0.6) × 10−3 105 – 107 This work
YES 2 × 104 3 × 10−10 ~ 5000 × 10−3 105 – 107 Acharyya et al. (2015)
YES 1 × 105 4 × 10−11 (10 – 100) × 10−3 105 – 107 Ruaud et al. (2015)
NO 6 × 104 3 × 10−10 ~ 40 × 10−3 ~ 105 Balucani et al. (2015)
NO 1 × 105 4 × 10−11 (2 – 10) × 10−3 105 – 106 Vasyunin & Herbst (2013)
YES 1 × 105 4 × 10−11 (0.3 – 50) × 10−3 105 – 106 Vasyunin & Herbst (2013)

Note. — The observed n(CH3O)/n(CH3OH) in B1-b is ~ 3 × 10−3 (Öberg et al. 2010; Cernicharo et al. 2012).