Table 3.

Kinematics information of 20 high-velocity post-AGB candidates.

vT*vφvRvzLzE
(km s−1)(km s−1)(km s−1)(km s−1)(kpc km s−1)(km2 s−2)
(1) IRAS 02143+5852>8.6
(2) IRAS 05089+0459>18.5
(3) IRAS 05208−203516.2216.313.0−4.91983.8−153156
(4) HD 4670366.5162.6−51.8−17.71857.2−149824
(5) HD 561265.1207.852.118.92104.9−148503
(6) IRAS 07140−232163.0240.1−11.9−3.82839.3−134521
(7) IRAS 07227−132015.0206.915.18.01992.9−152988
(8) IRAS 08187−190536.9207.3−8.7−1.02119.8−149469
(9) HD 116745185.4−84.6−56.6−74.8−541.3−184843
(10) IRAS 14325−6428207.3241.255.944.01457.7−167529
(11) IRAS 15210−6554>273.0
(12) HD 13756990.9226.4−50.2−79.31688.5−156543
(13) BD +33 2642238.313.5142.285.198.0−169581
(14) BD +32 275466.9159.420.912.81286.9−170975
(15) HD 161796109.6193.8−69.7−17.51551.1−161792
(16) BD −12 497027.0272.0-111.33.61706.0−154487
(17) IRAS 18075−0924>137.4
(18) HD 178443233.1−21.9−300.4−131.0−160.5−135111
(19) PHL 158047.6186.651.624.11495.6−165370
(20) LS III +52 579.77.033.3−42.057.6−181508
vT*vφvRvzLzE
(km s−1)(km s−1)(km s−1)(km s−1)(kpc km s−1)(km2 s−2)
(1) IRAS 02143+5852>8.6
(2) IRAS 05089+0459>18.5
(3) IRAS 05208−203516.2216.313.0−4.91983.8−153156
(4) HD 4670366.5162.6−51.8−17.71857.2−149824
(5) HD 561265.1207.852.118.92104.9−148503
(6) IRAS 07140−232163.0240.1−11.9−3.82839.3−134521
(7) IRAS 07227−132015.0206.915.18.01992.9−152988
(8) IRAS 08187−190536.9207.3−8.7−1.02119.8−149469
(9) HD 116745185.4−84.6−56.6−74.8−541.3−184843
(10) IRAS 14325−6428207.3241.255.944.01457.7−167529
(11) IRAS 15210−6554>273.0
(12) HD 13756990.9226.4−50.2−79.31688.5−156543
(13) BD +33 2642238.313.5142.285.198.0−169581
(14) BD +32 275466.9159.420.912.81286.9−170975
(15) HD 161796109.6193.8−69.7−17.51551.1−161792
(16) BD −12 497027.0272.0-111.33.61706.0−154487
(17) IRAS 18075−0924>137.4
(18) HD 178443233.1−21.9−300.4−131.0−160.5−135111
(19) PHL 158047.6186.651.624.11495.6−165370
(20) LS III +52 579.77.033.3−42.057.6−181508
*

Tangential velocity computed from the proper motion and parallax. In case the relative parallax measurement uncertainty is larger than |$20\%$|⁠, we provide 2σ lower limit.

Table 3.

Kinematics information of 20 high-velocity post-AGB candidates.

vT*vφvRvzLzE
(km s−1)(km s−1)(km s−1)(km s−1)(kpc km s−1)(km2 s−2)
(1) IRAS 02143+5852>8.6
(2) IRAS 05089+0459>18.5
(3) IRAS 05208−203516.2216.313.0−4.91983.8−153156
(4) HD 4670366.5162.6−51.8−17.71857.2−149824
(5) HD 561265.1207.852.118.92104.9−148503
(6) IRAS 07140−232163.0240.1−11.9−3.82839.3−134521
(7) IRAS 07227−132015.0206.915.18.01992.9−152988
(8) IRAS 08187−190536.9207.3−8.7−1.02119.8−149469
(9) HD 116745185.4−84.6−56.6−74.8−541.3−184843
(10) IRAS 14325−6428207.3241.255.944.01457.7−167529
(11) IRAS 15210−6554>273.0
(12) HD 13756990.9226.4−50.2−79.31688.5−156543
(13) BD +33 2642238.313.5142.285.198.0−169581
(14) BD +32 275466.9159.420.912.81286.9−170975
(15) HD 161796109.6193.8−69.7−17.51551.1−161792
(16) BD −12 497027.0272.0-111.33.61706.0−154487
(17) IRAS 18075−0924>137.4
(18) HD 178443233.1−21.9−300.4−131.0−160.5−135111
(19) PHL 158047.6186.651.624.11495.6−165370
(20) LS III +52 579.77.033.3−42.057.6−181508
vT*vφvRvzLzE
(km s−1)(km s−1)(km s−1)(km s−1)(kpc km s−1)(km2 s−2)
(1) IRAS 02143+5852>8.6
(2) IRAS 05089+0459>18.5
(3) IRAS 05208−203516.2216.313.0−4.91983.8−153156
(4) HD 4670366.5162.6−51.8−17.71857.2−149824
(5) HD 561265.1207.852.118.92104.9−148503
(6) IRAS 07140−232163.0240.1−11.9−3.82839.3−134521
(7) IRAS 07227−132015.0206.915.18.01992.9−152988
(8) IRAS 08187−190536.9207.3−8.7−1.02119.8−149469
(9) HD 116745185.4−84.6−56.6−74.8−541.3−184843
(10) IRAS 14325−6428207.3241.255.944.01457.7−167529
(11) IRAS 15210−6554>273.0
(12) HD 13756990.9226.4−50.2−79.31688.5−156543
(13) BD +33 2642238.313.5142.285.198.0−169581
(14) BD +32 275466.9159.420.912.81286.9−170975
(15) HD 161796109.6193.8−69.7−17.51551.1−161792
(16) BD −12 497027.0272.0-111.33.61706.0−154487
(17) IRAS 18075−0924>137.4
(18) HD 178443233.1−21.9−300.4−131.0−160.5−135111
(19) PHL 158047.6186.651.624.11495.6−165370
(20) LS III +52 579.77.033.3−42.057.6−181508
*

Tangential velocity computed from the proper motion and parallax. In case the relative parallax measurement uncertainty is larger than |$20\%$|⁠, we provide 2σ lower limit.

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