Chemistry and IR emission of acetylene in planet-forming regions of T Tauri disks - Impact of elemental abundances and dust properties

Open Access

Table A.1

Species included in the network with the c-C₃H₂ UV cross section.

nb C	Species
1	${C H}_{3}^{+}$ $Mathematical equation: $\[\mathrm{CH}_{3}^{+}\]$$
2	$C_{2}^{+}, C_{2} N$ $Mathematical equation: $\[\mathrm{C}_{2}^{+}, \mathrm{C}_{2} \mathrm{N}\]$$
3	CH₂CCH₂, CH₃CCH, CH₃CHCH₂, C₃H₅
4	CH₂CHCCH, C₄H₃, CH₂CHCHCH₂, C₄H₂^a
5	C₃CCH, C₅, C₅H₂, C₅H₅, C₅H₆, CH₃C₄H, H₂CCCHCCH, C₃HCCH

Notes. ^(a)C₄H₂ has the C₄H cross section.

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