Table 1.

The molecular clouds around the SS 433/W 50 system identified by previous studies.*

VLSRDistance
Name(km s−1)(kpc)References
S142.93.01
S245.43.01
S344.13.01
S443.23.01
S544.83.01
S642.13.01
N155.83.51, 2, 3
N253.73.51, 2, 3
N353.03.51, 2, 3
N449.43.51, 3
G39.315−1.155734.94
G40.331−4.302744.94
VLSRDistance
Name(km s−1)(kpc)References
S142.93.01
S245.43.01
S344.13.01
S443.23.01
S544.83.01
S642.13.01
N155.83.51, 2, 3
N253.73.51, 2, 3
N353.03.51, 2, 3
N449.43.51, 3
G39.315−1.155734.94
G40.331−4.302744.94
*

Column 1: Name of each molecular cloud. Column 2: Peak velocity. Column 3: Kinematic distance referred to in each paper. Note that the values of N1 to N4 refer to reference 1. Column 4: References—(1) Yamamoto et al. (2008), (2) Liu et al. (2020), (3) Yamamoto et al. (2022), (4) Su et al. (2018).

Table 1.

The molecular clouds around the SS 433/W 50 system identified by previous studies.*

VLSRDistance
Name(km s−1)(kpc)References
S142.93.01
S245.43.01
S344.13.01
S443.23.01
S544.83.01
S642.13.01
N155.83.51, 2, 3
N253.73.51, 2, 3
N353.03.51, 2, 3
N449.43.51, 3
G39.315−1.155734.94
G40.331−4.302744.94
VLSRDistance
Name(km s−1)(kpc)References
S142.93.01
S245.43.01
S344.13.01
S443.23.01
S544.83.01
S642.13.01
N155.83.51, 2, 3
N253.73.51, 2, 3
N353.03.51, 2, 3
N449.43.51, 3
G39.315−1.155734.94
G40.331−4.302744.94
*

Column 1: Name of each molecular cloud. Column 2: Peak velocity. Column 3: Kinematic distance referred to in each paper. Note that the values of N1 to N4 refer to reference 1. Column 4: References—(1) Yamamoto et al. (2008), (2) Liu et al. (2020), (3) Yamamoto et al. (2022), (4) Su et al. (2018).

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