Table 4: Global fluxes and scale lengths in BIMA SONG sources.
Galaxy S1.4 S60 $S_{\rm CO}$ Referencea $l_{\rm CO}^{b}$ $l_{\rm RC}^{c}$ $l_{\rm CO}$/ $l_{\rm RC}$
  (mJy) (Jy) (Jy km s-1)   (kpc) (kpc)  
IC 342 2475 255.96 20 000 1, 2, 3 $3.5 \pm 0.2$ $6.21 \pm 0.06$ 0.56
NGC 0628 180 20.86 1514 2 $3.2 \pm 0.1$ $15.3 \pm 0.1$ 0.21
NGC 1068 4991 181.95 4102   $1.6 \pm 0.4$ $0.7 \pm 0.2$ 2.16
NGC 2903 407 60.03 3254   $2.0 \pm 0.2$ $1.7 \pm 0.2$ 1.21
NGC 3351 48 19.92 1513   - - -
NGC 3521 357 47.02 4800   $2.1 \pm 0.2$ $4.1 \pm 0.1$ 0.52
NGC 3627 458 67.8 4259   $5.1 \pm 0.1$ $3.5 \pm 0.1$ 1.45
NGC 3938 62 9.24 923   $4.0 \pm 0.2$ $6.3 \pm 0.1$ 0.64
NGC 4258 792 21.60 2686 1, 2 $2.1 \pm 0.2$ $3.1 \pm 0.3$ 0.70
NGC 4303 416 37.53 2427   $3.2 \pm 0.1$ $3.3 \pm 0.1$ 0.96
NGC 4321 340 25.86 2972   $4.8 \pm 0.1$ $5.0 \pm 0.1$ 0.96
NGC 4414 231 30.11 2453   $3.4 \pm 0.2$ $3.00 \pm 0.03$ 1.13
NGC 4569 83 10.08 1096   $2.6 \pm 0.1$ $2.5 \pm 0.2$ 1.04
NGC 4736 254 69.2 2641   $0.9 \pm 0.4$ $0.7 \pm 0.2$ 1.22
NGC 4826 103 35.45 1845   $0.6 \pm 1.1$ $0.4 \pm 0.7$ 1.46
NGC 5005 176 22.3 1278   $2.9 \pm 0.3$ $3.2 \pm 0.1$ 0.90
NGC 5033 178 16.45 2469   $4.5 \pm 0.1$ $3.2 \pm 0.1$ 1.39
NGC 5055 390 40.02 3812   $2.4 \pm 0.1$ $2.3 \pm 0.1$ 1.03
NGC 5194 1490 98.8 10 097   $2.9 \pm 0.1$ $3.4 \pm 0.1$ 0.84
NGC 5247 53 8.07 1102 4, 5 $7.1 \pm 0.2$ $7.3 \pm 0.1$ 0.97
NGC 5248 140 20.71 1829   $3.0 \pm 0.3$ $4.2 \pm 0.1$ 0.72
NGC 5457 750 88.04 3479   - - -
NGC 6946 1395 136.69 9273 2, 4 $2.5 \pm 0.2$ $3.83 \pm 0.04$ 0.65
NGC 7331 373 35.29 2762 2, 4 $3.2 \pm 0.1$ $3.33 \pm 0.03$ 0.96
Average             $0.98\pm 0.41$
a Flux references: (1) S1.4 is 1.4 GHz RC from White & Becker (1992); (2) S60 is 60 $\mu$m emission from Rice et al. (1988); (3) $S_{\rm CO}$ from Crosthwaite et al. (2001); (4) S 1.4 from Condon (1987); (5) S 60, S100 from IRAS Faint Source Catalog; if not otherwise indicated, S1.4 is from Condon et al. (1990), S60 is from the IRAS Bright Galaxy Sample, Soifer et al. (1989); and $S_{\rm CO}$ is from Helfer et al. (2003).
b CO scale lengths modeled from the 55 $^{\prime \prime }$ 12 m data.
c RC scale lengths modeled from the low-resolution RC data from either the present study or from NVSS imaging.


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