Table 5
Source distancesa.
Field/ | d near | d far | R GC | Remarkc |
clumpb | [kpc] | [kpc] | [kpc] | |
|
||||
G1.87-0.14 | (![]() |
![]() |
2.19 | dfar for the whole field |
G2.11+0.00 |
![]() |
![]() |
2.90 | dnear for all clumps except SMM 5 |
SMM 5 |
![]() |
![]() |
1.04 | |
G11.36+0.80 |
![]() |
![]() |
5.23 | |
G13.22-0.06 |
![]() |
![]() |
5.02 | this dnear was not used for any of the clumps |
SMM 5 |
![]() |
![]() |
4.38 | dnear also for SMM 2, 4, 6, 7, 9, 11, 12 |
SMM 10 |
![]() |
![]() |
4.32 | dnear also for SMM 1, 3, 8 |
SMM 13 |
![]() |
![]() |
6.52 | |
SMM 17 |
![]() |
![]() |
5.00 | dnear also for SMM 15, 20 |
SMM 24 | (![]() |
![]() |
4.61 | dfar also for SMM 26, 33, 34 |
SMM 25 |
![]() |
![]() |
4.17 | dnear also for SMM 18, 21 |
SMM 27 |
![]() |
![]() |
5.00 | dnear also for SMM 22, 23 |
SMM 28 |
![]() |
![]() |
4.19 | dnear also for SMM 14, 16, 19, 30, 31 |
SMM 29 | (![]() |
![]() |
4.57 | |
SMM 32 |
![]() |
![]() |
4.23 |
Notes.
The near and far kinematic distances were determined using the Reid et al. (2009) rotation curve of the Galaxy. The near distance was adopted unless otherwise stated.
The fields G2.11 and G13.22 are known to contain sources at different distances than determined here from our C17O radial velocities (see text).
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