Table 6: Continuum observations and derived properties (dust temperature, C18O column density, CO depletion factor) for sources in our survey.

Source		 IRAS F(60 $\mu$m) F(100 $\mu$m) Wavelength of additional data $T_{\rm Dust}$ N(C18O) $f\rm _D$(CO)
    [Jy] [Jy] [$\mu$m] [K] [cm-2]  
L 1448 IRS 2 03222+3034 14.3 <169 450, 850, 11001,3 27 $6.07\times 10^{15}$ $2.6\pm 0.6$
L 1448 IRS 3 03225+3034 25.1 169 11003 27 $1.08\times 10^{16}$ $4.4\pm 1.0$
L 1448 C F03226+3033 53.4 355 450, 850, 11002,3 32 $7.18.19\times 10^{15}$ $2.8\pm 0.6$
L 1455 A1 03245+3002 47.1 93.6 1100, 450, 8503,5 37 $3.53\times 10^{15}$ $1.5\pm 0.4$
L 1455 A2 F03247+3001 66.4 206 - 30 $1.83\times 10^{15}$ -
Per 4 S - - - 11003 - $3.18\times 10^{15}$ -
Per 4 N 03262+3123 1.07 <12.4 11003 23 $2.18\times 10^{15}$ $2.4\pm 0.11$
Per 5 03267+3128 1.88 <10.4 11003 26 $3.28\times 10^{15}$ $1.6\pm 0.4$
Per 6 03271+3013 7.53 8.19 - 45 $ 4.28\times 10^{15}$ -
IRAS 03282 03282+3035 2.33 13.9 450, 850, 11002,3 23 $3.28\times 10^{15}$ $3.9\pm 0.9$
Barnard 1-B 03301+3057 <6.18 35.5 1100, 8503,4 18 $1.16\times 10^{16}$ $2.9\pm 0.7$
HH 211 03407+3152 <2.06 <30.8 1100, 450, 8503,5 <21 $8.21\times 10^{15}$ $2.9\pm 0.7$
Barnard 5 IRS 1 03445+3242 15.5 15.4 11003 50 $1.23\times 10^{16}$ $0.3\pm 0.09$
L 1527 04368+2557 17.8 73.3 450, 850, 13002 27 $7.75\times 10^{15}$ $2.3\pm 0.5$
L 483 18148-0440 89.1 166 450, 8502 34 $ 1.15\times 10^{16}$ $2.1\pm 0.5$
SMM 5 - - - - - $9.70\times 10^{15}$ -
L 723 19156+1906 6.93 20.7 450, 8502 25 $4.36\times 10^{15}$ $2.9\pm 0.7$
L 673 A 19180+1114 2.55 10.6 - 28 $4.47\times 10^{15}$ -
B 335 19345+0727 8.3 42 450, 850, 13002 27 $4.41\times 10^{15}$ $3.3\pm 0.8$
L 1157 20386+6751 10.9 43.5 1300, 450, 8502,5 30 $3.19\times 10^{15}$ $4.2\pm 1.0$
The errors in the dust temperatures are $\sim$2 K, and the C18O column densities are accurate to 10%.
References: 1 O'Linger et al. (1999); 2 Shirley et al. (2000); 3 Enoch et al. (2006); 4 Hatchell et al. (2005); 5 Froebrich et al. (2003).

Source LaTeX | All tables | In the text