Table 2: Results for Henize 2-10.
Henize 2-10            
Transition Freq. Beam size $\int(T_{\rm mb}{\rm d}v)$ Intensity Flux Referencesa
  (GHz) ( $\hbox{$^{\prime\prime}$ }$) (K km s-1) (W m-2 sr-1) (W m-2)  
CI(3P1-3P0) 492.162 14.55 $4.2\pm 0.8$ $5.1\times10^{-10}$ $3.0\times10^{-18}$ 4 and 5b
    21.90 $2.5\pm0.5$ $3.0\times10^{-10}$ $3.8\times10^{-18}$ 4 and 5b
12CO(1-0) 115.271 40.00 $10.0\pm0.8$ $1.6\times10^{-11}$ $6.7\times10^{-19}$ 1
    21.90 $27.3\pm2.2$ $4.3\times10^{-11}$ $5.5\times10^{-19}$ 1
    55.00 $4.9\pm0.2$ $7.6\times10^{-12}$ $6.1\times10^{-19}$ 2
    21.90 $23.9\pm1.0$ $3.7\times10^{-11}$ $4.8\times10^{-19}$ 2*
12CO(2-1) 230.538 21.00 $17.3\pm1.4$ $2.2\times10^{-10}$ $2.5\times10^{-18}$ 1*
    27.00 $6.8\pm0.8$ $8.5\times10^{-11}$ $1.7\times10^{-18}$ 2
    21.90 $9.4\pm1.1$ $1.2\times10^{-10}$ $1.5\times10^{-18}$ 2
12CO(3-2) 345.796 21.90 $11.5\pm2.3$ $4.9\times10^{-10}$ $6.2\times10^{-18}$ 5*
    21.00 $23.2\pm2.1$ $9.8\times10^{-10}$ $1.2\times10^{-17}$ 1
    22.00 $16.6\pm0.6$ $7.0\times10^{-10}$ $9.0\times10^{-18}$ 3
12CO(4-3) 461.041 14.55 $18.6\pm4.2$ $1.9\times10^{-9}$ $1.1\times10^{-17}$ 5
    21.90 $10.9\pm2.4$ $1.1\times10^{-9}$ $1.4\times10^{-17}$ 5*
12CO(6-5) 691.473 10.60 $15.7\pm3.1$ $5.3\times10^{-9}$ $1.6\times10^{-17}$ 5
    21.90 $6.8\pm1.3$ $2.3\times10^{-9}$ $2.9\times10^{-17}$ 5*
12CO(7-6) 806.652 8.95 $15.2\pm3.0$ $8.2\times10^{-9}$ $1.7\times10^{-17}$ 5
    21.90 $5.8\pm1.2$ $3.1\times10^{-9}$ $4.0\times10^{-17}$ 5*
13CO(1-0) 110.201 40.00 <0.5 < $6.8\times10^{-13}$ < $2.9\times10^{-20}$ 1
    21.90 <1.4 < $1.8\times10^{-12}$ < $2.4\times10^{-20}$ 1
    57.00 $0.3\pm0.1$ $3.9\times10^{-13}$ $3.4\times10^{-20}$ 2
    21.90 $1.6\pm0.5$ $2.2\times10^{-12}$ $2.8\times10^{-20}$ 2*
13CO(2-1) 220.399 21.00 $0.9\pm0.2$ $9.9\times10^{-12}$ $1.2\times10^{-19}$ 1*
13CO(3-2) 330.588 14.00 $2.3\pm0.6$ $8.5\times10^{-11}$ $4.4\times10^{-19}$ 1
    21.90 $1.3\pm0.3$ $4.8\times10^{-11}$ $6.1\times10^{-19}$ 1*
    21.90 $1.8\pm0.5$ $6.7\times10^{-11}$ $8.5\times10^{-19}$ 5
a References: 1: Baas et al. (1994); 2: Kobulnicky et al. (1995); 3: Meier et al. (2001); 4: Gerin & Phillips (2000); 5: this work; *: used for models.
b We analysed again spectra from Gerin & Phillips (2000).


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