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Table 2:

Results from HARP-B (HCO+ 4-3 and C18O 3-2), APEX-2a (HCO+ 4-3) and RxB (C18O 3-2) observations at the source position.
Source HCO+ 4-3a   C18O 3-2   Notes
  $\int$ $T_{{\rm MB}}$ dV $T_{{\rm MB}}$ $\int$ $T_{{\rm MB}}$ dV $T_{{\rm MB}}$  
  [K km s-1] [K] [K km s-1] [K]  
C2D-162527.6 - <0.09 - - See Fig. 5
GSS 26 - - - - See Fig. 9
CRBR 2315.8-1700 6.3 5.2* - - See Fig. 5
CRBR 2317.3-1925 1.5b 2.0b - - See Fig. 9
VSSG 1 - <0.4 - - See Fig. 9
GSS 30 16.7 9.1 10.7c 6.3c See Figs. 2 and 10
LFAM 1 18.4 10.8 - - See Figs. 2 and 10, GSS 30 maps
CRBR 2324.1-1619 - - 14.5 12.2 See Figs. 2 and 10, VLA1623 maps
VLA 1623 16.2 9.0 10.4 17.9d See Figs. 2 and 10
GY51 - - - - See Fig. 9
CRBR 2339.1-2032 0.55 0.45* - - See Fig. 5
WL 12 0.87 1.4 4.8 3.9 See Figs. 3 and 10
WL 2 0.3 0.18* - - See Fig. 5
LFAM 26 1.95 1.8 6.4 3.3 See Fig. 3
WL 17 0.6 0.45 - - See Fig. 4
Elias 29 4.5b 2b 10.4e 4.3e See Fig. 4, WL17 map and Figs. 9 and 10
GY 224 - <0.27b - - See Fig. 9
WL19 - < 0.1 6.3 4.5 See Fig. 4
WL 20S - <0.26b 5.0c 2.3c See Fig. 10
IRS 37 3.7 2.5 9.55 5.7 See Fig. 3
WL 3 3.7 2.2 8.8 6.3 See Fig. 3, IRS 37 map
IRS 42 0.45 0.7* 4.0 1.2* See Fig. 4
WL 6 0.92 0.6 5.25 4.5* See Figs. 9 and 10
GY 256 0.75 0.45* 5.4 4.5* See Figs. 9 and 10, WL6 maps
IRS 43 4.5d 1.6d 6.5c 3.2c See Figs. 2, 9 and 10
IRS 44 3.4d 0.5d 5.8 2.8 See Fig. 3
Elias 32 5.6 4.3 3.1c 4.5c See Figs. 2 and 10, Elias 33 maps
Elias 33 6.3 5.7 6.0c 3.0c See Figs. 2 and 10
IRS 48 - <0.09 2.6 2.3 See Fig. 4
GY 312 - <0.1 - - See Fig. 5
IRS 51 0.75 0.75 2.0 2.8* See Figs. 4 and 10
C2D-162741.6 - <0.1 - - See Fig. 5
C2D-162748.1 - <0.34b - - See Fig. 9
IRS 54 0.53 0.45 3.4 3.3 See Fig. 3
IRAS 16285-2355 2.1 3.0 2.3 3.0 See Fig. 3
C2D-162857.9 - <0.34b - - See Fig. 9
IRS 63 0.75 1.2 1.7 3.3 See Fig. 4
Disks
Haro 1-4 - <0.29b - - See Fig. 9
DoAR 25 - <0.28b - - See Fig. 9
OphE MM3 1.7 1.6* 5.5 3.0* See Fig. 3, LFAM 26 map
SR 21 - <0.28b - - See Fig. 9
CRBR 2422.8-3423 1.9 1.4* - - See Fig. 2, IRS 43 map, and Fig. 4, NW corner of IRS 42
IRS 46 - <0.09 2.9 2.1 See Fig. 3, IRS 44 map
SR 9 - <0.24b - - See Fig. 9
2Mass 16282 - <0.35b - - See Figs. 9 and 10
a Intensities marked with a * do not peak at source position.
b APEX-2a receiver. Upper limits (2$\sigma$) in 0.4 km s-1 bin.
c JCMT RxB data.
d Outflowing gas detected (width $\sim$20 km s-1).
e C18O data taken from Boogert et al. (2002), obtained with the CSO.

Source LaTeX | All tables | In the text

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