Table 2
LOS velocities of the M8 clumps.
Clump | v1,LSR | v2,LSR |
---|---|---|
(km s−1) | (km s−1) | |
HG | 9.75 | 5.87 |
WC1 | 8.09 | − |
WC2 | 8.48 | − |
WC3* | 10.40 | − |
WC4 | 11.53 | − |
WC5 | 9.89 | 7.96 |
WC6 | 9.59 | 7.79 |
WC7 | 12.61 | 9.29 |
WC8 | 9.25 | − |
WC9 | 9.65 | − |
SW1 | 8.95 | 11.30 |
EC1 | 14.97 | 12.68 |
EC2 | 12.35 | 15.43 |
EC3 | 12.64 | 16.21 |
EC4 | 16.61 | − |
EC5 | 16.90 | − |
E | 10.73 | − |
SE1 | 13.53 | − |
SE2 | 13.78 | 17.47 |
SE3 | 12.70 | − |
SE4 | 12.24 | − |
SE5 | 12.12 | − |
SE6 | 10.71 | − |
SE7 | 9.95 | - |
SE8* | 10.83 | − |
SC1 | 9.84 | − |
SC2 | 9.82 | 8.80 |
SC3 | 9.94 | 8.97 |
SC4 | 12.49 | 10.64 |
SC5* | 12.55 | 11.16 |
SC6 | 12.32 | − |
SC7 | 11.24 | 13.78 |
SC8 | 12.50 | − |
SC9 | 13.25 | − |
C1 | 13.88 | 9.67 |
C2 | 12.24 | 10.55 |
C3 | 15.60 | − |
Notes. These values are based on the line profiles of the 18CO (2−1) and 17CO (2−1) transitions. The clumps marked with a* have been observed at deviating coordinates with APEX and the IRAM 30m telescope. The table lists the LOS velocities on the position observed with the IRAM 30m telescope based on the 18CO and 17CO transitions with J = 1−0.
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