C6H2+
Triacetylene ion
Flags: RATE12
Empirical: C6H2+
Mass: 74 amu
Heat of formation: 1569.0 kJ mol-1
Added to system: 2003-05-06 06:43:21
Reactions: Formation | Destruction
24 C6H2+ formation reactions
Reaction | α | β | γ | Tl - Tu (K) | |
---|---|---|---|---|---|
1 | C2H2+ + C6H2 → C6H2+ + C2H2 | 5.00e-10 | -0.50 | 0.00 | 10 - 300 |
2 | H+ + C6H2 → C6H2+ + H | 2.00e-9 | -0.50 | 0.00 | 10 - 300 |
3 | C+ + CH3C4H → C6H2+ + H2 | 7.50e-10 | 0.00 | 0.00 | 10 - 41000 |
4 | C2H2+ + C4H → C6H2+ + H | 1.00e-9 | -0.50 | 0.00 | 10 - 41000 |
5 | C2H2+ + HC4H → C6H2+ + H2 | 1.00e-17 | 0.00 | 0.00 | 10 - 41000 |
6 | C2H2 + C4H+ → C6H2+ + H | 1.50e-9 | 0.00 | 0.00 | 10 - 41000 |
7 | C2H3+ + C4H → C6H2+ + H2 | 4.00e-10 | -0.50 | 0.00 | 10 - 41000 |
8 | C2H3+ + C6H → C6H2+ + C2H2 | 5.00e-10 | -0.50 | 0.00 | 10 - 41000 |
9 | C2H4+ + C5H → C6H2+ + CH3 | 2.10e-9 | -0.50 | 0.00 | 10 - 41000 |
10 | C2H + C4H2+ → C6H2+ + H | 1.30e-9 | 0.00 | 0.00 | 10 - 41000 |
11 | C3H2+ + C3H2 → C6H2+ + H2 | 1.00e-9 | -0.50 | 0.00 | 10 - 41000 |
12 | C3H2+ + H2CCC → C6H2+ + H2 | 1.00e-9 | -0.50 | 0.00 | 10 - 41000 |
13 | C3H + C3H2+ → C6H2+ + H | 2.50e-9 | -0.50 | 0.00 | 10 - 41000 |
14 | C3H + C3H3+ → C6H2+ + H2 | 1.50e-9 | -0.50 | 0.00 | 10 - 41000 |
15 | C3H + CH2CCH+ → C6H2+ + H2 | 1.50e-9 | -0.50 | 0.00 | 10 - 41000 |
16 | C4H2+ + HC4H → C6H2+ + C2H2 | 1.30e-10 | 0.00 | 0.00 | 10 - 41000 |
17 | C + C5H3+ → C6H2+ + H | 5.00e-10 | 0.00 | 0.00 | 10 - 300 |
18 | CH3+ + C5H → C6H2+ + H2 | 3.20e-9 | -0.50 | 0.00 | 10 - 41000 |
19 | CH4 + C5+ → C6H2+ + H2 | 9.68e-11 | 0.00 | 0.00 | 10 - 41000 |
20 | H2 + C6H+ → C6H2+ + H | 1.30e-12 | 0.00 | 0.00 | 10 - 41000 |
21 | H3+ + C6H → C6H2+ + H2 | 2.50e-9 | -0.50 | 0.00 | 10 - 41000 |
22 | HCO+ + C6H → C6H2+ + CO | 2.00e-9 | -0.50 | 0.00 | 10 - 41000 |
23 | C6H2 + PHOTON → C6H2+ + e- | 2.00e-10 | 0.00 | 2.50 | 10 - 41000 |
24 | H2 + C6+ → C6H2+ + PHOTON | 5.20e-14 | -0.50 | 0.00 | 10 - 300 |
Variation of log fractional abundance (relative to H2) with log time (years) in a dark cloud model. Ref. RATE12 paper.