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Table B.5
Sample of rotating spheroidals in the Virgo cluster.
| Name | M R | i |
|
R d | Ref. | v R d | v last | R last |
|
Ref. | V R d | V last | VRd/Rd |
| (mag) | (°) | (mag/′′2) | (kpc) | (km s-1) | (km s-1) | (kpc) | (km s-1) | (km s-1) | (km s-1) | (km s-1/kpc) | |||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) | (13) | (14) |
|
|
|||||||||||||
| VCC 178 | −16.6 ± 0.2 | 60 ± 3 | 20.9 ± 0.1 | 0.52 | a | 14 ± 3 | 30 ± 3 | 1.1 | 46 ± 5 | b | 48 ± 5 | 73 ± 7 | 92 ± 12 |
| VCC 437 | −18.1 ± 0.2 | 54 ± 3 | 21.7 ± 0.1 | 1.60 | a | 49 ± 5 | 49 ± 5 | 1.6 | 50 ± 5 | b | 70 ± 5 | 70 ± 5 | 44 ± 5 |
| VCC 543 | −17.9 ± 0.2 | 62 ± 3 | 21.6 ± 0.1 | 1.23 | a | 35 ± 4 | 46 ± 4 | 1.6 | 44 ± 5 | b | 56 ± 5 | 68 ± 5 | 45 ± 5 |
| VCC 990 | −17.6 ± 0.2 | 50 ± 3 | 20.0 ± 0.1 | 0.53 | a | 18 ± 3 | 43 ± 3 | 1.3 | 43 ± 5 | b | 46 ± 5 | 80 ± 7 | 87 ± 11 |
| VCC 1036 | −18.3 ± 0.2 | 69 ± 3 | 21.4 ± 0.2 | 1.32 | a | 32 ± 2 | 52 ± 2 | 2.1 | 37 ± 4 | b | 49 ± 3 | 70 ± 4 | 37 ± 4 |
| VCC 1122 | −17.3 ± 0.2 | 70 ± 3 | 21.5 ± 0.2 | 0.90 | a | 17 ± 3 | 28 ± 3 | 1.4 | 40 ± 4 | b | 43 ± 4 | 57 ± 5 | 48 ± 6 |
| VCC 2019 | −17.6 ± 0.2 | 47 ± 3 | 20.6 ± 0.1 | 0.73 | a | 28 ± 3 | 42 ± 3 | 1.1 | 41 ± 4 | b | 50 ± 4 | 65 ± 4 | 68 ± 8 |
| VCC 2050 | −16.8 ± 0.2 | 66 ± 3 | 21.3 ± 0.2 | 0.62 | a | 11 ± 3 | 20 ± 3 | 1.0 | 37 ± 6 | b | 39 ± 6 | 51 ± 7 | 60 ± 10 |
Notes. We assumed a distance of 16.1 ± 1.2 Mpc for all galaxies.
Reference. (a) van Zee et al. (2004a); (b) van Zee et al. (2004b).
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