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Christopher added V > 1 [1].tex
almost 10 years ago
Commit id: 5dcbfb8013d0c40a3ad03571f02e4d3799a26de0
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During the main time period of the outflow (0.2 - 0.3Myr), all observations slightly underestimate the due to optical thickness. However, the observations with a higher velocity cutoff are not optically thinner than those with a lower one. Gas with V > 1 is as optically thin as we can get.
At later times, we are missing a lot of the mass in the 1 < V < 2 band, but this is likely an issue with the integrated emission. As we can see when comparing to the density data (with the true mass), the integrated emission overestimates this mass.
