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Table 1

Main parameters considered in our modeling.

nH (cm−3) AV (mag) tcold (a) (yr) twarmup (a) (yr) Tmax (a) (K) Tgas (b) (K) Tdust (b) (K) χ (c) G0 (c) ζCR (d) (s−1) (d)
1 1 1.3 × 10−17 10−4
2 × 103 (e,f) 2 1 × 105 1 × 103 10 10 10 10 10 1.3 × 10−16 10−3
2 × 104 5 2 × 105 1 × 104 20 20 20 (g) 102 102 1.3 × 10−15 10−2
2 × 105 10 (h) 3 × 105 (h) 5 × 104 30 30 30 103 103 1.3 × 10−14 10−1
2 × 106 25 4 × 105 1 × 105 50 50 104 104 (i) 1.3 × 10−13 (j) 1
2 × 107 50 5 × 105 2 × 105 (k) 70 65 (g)
102 6 × 105 3 × 105 100 100
103 7 × 105 4 × 105 150
8 × 105 5 × 105 200 (k)
9 × 105 6 × 105 300
1 × 106 7 × 105 400
8 × 105 500
9 × 105 700
1 × 106 1000

Notes. (a) tcold, twarmup, and Tmax are time spans of the cold and warm-up phases and maximum temperature that are used in the evolving physical models. (b) Tgas and Tdust are gas and dust temperatures that are used in the static models. (c) χ and G0 are used to calculate the rate coefficients of photodissociation and photodesorption induced by UV photons, respectively. (d) ζCR and are used to calculate the rate coefficients of photodissociation and photodesorption induced by cosmic ray particles, respectively. (e) Boldface indicates the fiducial values adopted in our simulations.

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