Table 3
Median and 90% confidence limits from different analysis strategies.
| Strategy | V200 | V300 | ||||
| νesc(R0) | M 340,NFW | M 340,contr | νesc(R0) | M 340,NFW | M 340,contr | |
| (km s-1) | (1012 M⊙) | (1012 M⊙) | (km s-1) | (1012 M⊙) | (1012 M⊙) | |
|
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| Estimates considering the RAVE and B00 data; VLSR = 220 km s-1. | ||||||
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| Binned |
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| Localized |
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| Estimates considering the RAVE data only; VLSR = 220 km s-1. | ||||||
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| Binned |
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| Localized |
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|
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| Estimates considering the RAVE and B00 data; VLSR = 240 km s-1. | ||||||
|
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| Binned |
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| Localized |
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| Estimates considering the RAVE data only; VLSR = 240 km s-1. | ||||||
|
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| Binned |
|
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|||
| Localized |
|
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|
|
|
|
Notes. The masses M340,NFW are estimated assuming an NFW profile for the dark matter halo, and the masses M340,contr are based on an adiabatically contracted NFW profile. In the lower part of the table we show the results if we assume a different VLSR to facilitate a comparison to other estimates based on this alternative value.
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