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Table 3
Outflow results from kinematic analysis.
G28.2-0.04 | NGC 7538 IRS 1 | |||
(tdyn = 2.4 × 104 yr) | (tdyn = 4.2 × 104 yr) | |||
Blue | Red | Blue | Red | |
(Δv = −10, − 3) | (Δv = 3,10) | (Δv = −20, − 10) | (Δv = 10,20) | |
|
||||
Ma | 0.89 | 1.60 | 0.43 | 0.98 |
Pb | 8.3 | 8.7 | 4.6 | 10.7 |
Ec | 7.6 | 4.9 | 4.9 | 11.8 |
Ld | 0.30 | 0.20 | 0.10 | 0.23 |
Ṁe | 3.6 | 6.4 | 1.0 | 2.3 |
Notes. A calibration uncertainty of 20% is not propagated through these equations. The velocity ranges listed above each column (Δv) represent the integration limits with respect to the VLSR stated in Table 1.
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