Table 3: We give the air wavelengths, upper energy levels, Eistein A coefficients and degeneracies of the H2 lines detected in IRAS 19410+2336.
Transition $\lambda_j$ Ej Aj gj
  ($\mu $m) (K) (10-7 s)  
1-0 S(3) 1.9571 8365 4.21 33
1-0 S(2) 2.0332 7584 3.98 9
3-2 S(5) 2.0650 20 856 4.53 45
2-1 S(3) 2.0729 13 890 5.77 33
1-0 S(1) 2.1212 6956 3.47 21
3-2 S(4) 2.1274 19 912 5.25 13
2-1 S(2) 2.1536 13 152 5.60 9
3-2 S(3) 2.2008 19 086 5.63 33
1-0 S(0) 2.2229 6471 2.53 5
2-1 S(1) 2.2471 12 550 4.98 21
2-1 S(0) 2.3549 12 095 3.68 5
3-2 S(1) 2.3857 17 818 5.15 21


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