ΔRw values needed to have NH,meas = NH,pred with the assumption of all obscuration due to a warp of the maser disk entering the line of sight.
|Name||Rw [pc]||ΔRw [pc]|
Notes. Uncertainties are neglected for clarity. Warp depths are lower than, or comparable to, the uncertainties on outer maser radii. The five sources with a lower limit on the column density consequently have a lower limit on the warp depth.
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