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)

U_S V_S W_S 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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