Adopted components of the solar motion and velocity dispersions

Adopted components of the solar motion and velocity dispersions

Table
Adopted components of the solar motion and
velocity dispersions
type       solar motion (km/sec) spread in velocities (km/sec)
US VS WS U V W
cO–cB5 –9.0 +13.4 +3.7 12 11   9
cF–cM –7.9 +11.7 +6.5 13   9   7
gA –13.4 +11.6 +10.3 22 13   9
gF –19.7 +18.5 +9.5 28 15   9
gG –7.2 +11.1 +6.9 26 18 15
gK0 –10.6 +18.6 +6.5 31 21 16
gK3 –9.0 +17.6 +6.4 31 21 17
gM –4.5 +18.3 +6.2 31 23 16
carbon stars –10.7 +31.8 +3.5 48 23 16
subgiants –8.0 +28.0 +8.0 43 27 24
B0 –9.6 +14.5 +6.7 10   9   6
dA0 –7.3 +13.7 +7.2 15   9   9
dA5 –8.5 +7.8 +7.4 20   9   9
dF5 –10.1 +12.3 +6.2 27 17 17
dG0 –14.5 +21.1 +6.4 26 18 20
dG5 –8.1 +22.1 +4.3 32 17 15
dK0 –10.8 +14.9 +7.4 28 16 11
dK5 –9.5 +22.4 +5.8 35 20 16
dM0 –6.1 +14.6 +6.9 32 21 19
dM5 –9.8 +19.3 +8.6 31 23 16
white dwarfs (white dwarf star) –6    +37    +8    50 33 25
planetary nebulae (planetary nebula) –8    +29    +8    45 35 20
classical Cepheids (Cepheid variable) –8.6 +12.0 +7.6 13   9   5
interstellar Ca II –11.4 +14.4 +8.2   6
See as table:

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Universalium. 2010.

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