t1 cols ['ALMAGAL', 'ID', 'GLON', 'GLAT', 'VLSR', 'Dist', 'Mass', 'Lum', 'ModelTemp', 'Class', '_RA.icrs', '_DE.icrs']
t2 cols ['ID', 'Xoffset', 'Yoffset', 'FlowRateLout', 'FlowRateLin', 'FlowRateRin', 'FlowRateRout', 'Masscore', 'Idx']
t2 FlowRateLin: unit=0.0001 solMass / yr desc=Inner left flowrate
t2 FlowRateRin: unit=0.0001 solMass / yr desc=Inner right flowrate

=== Total large-scale inflow rate Mdot (Msun/yr) by evolutionary class ===
  Quiescent     N=17  median=5.39e-01  q25-75=2.5e-01-1.9e+00  max=1.0e+01
  Protostellar  N=23  median=1.60e+00  q25-75=9.4e-01-7.2e+00  max=2.0e+01
  YSO           N=22  median=6.55e+00  q25-75=3.3e+00-1.5e+01  max=6.9e+01
  HII Region    N=25  median=6.92e+00  q25-75=2.7e+00-1.3e+01  max=8.6e+01

=== Fraction of each class with a detected accretion flow ===
  Quiescent     17/17 (100%)
  Protostellar  23/23 (100%)
  YSO           22/22 (100%)
  HII Region    25/25 (100%)

=== Our RMS HII regions in Wells: measured inflow ===
  AG025.8012-0.1563      Class=HII Region   Mdot=2.4739999771118164
  AG024.5073-0.2196      Class=HII Region   Mdot=2.0620000064373016
  AG029.9558-0.0161      Class=HII Region   Mdot=85.5540018081665
  AG030.2960+0.0554      Class=HII Region   Mdot=11.21400000154972
  AG305.1957+0.0330      Class=HII Region   Mdot=7.220999836921692
  AG308.6467+0.6472      Class=HII Region   Mdot=4.954999923706055
  AG309.9212+0.4780      Class=HII Region   Mdot=43.98899841308594
  AG311.6268+0.2907      Class=HII Region   Mdot=25.86300027370453
  AG316.8113-0.0575      Class=HII Region   Mdot=29.26900005340576
  AG320.6753+0.2459      Class=HII Region   Mdot=3.3129999339580536
  AG327.4026+0.4445      Class=HII Region   Mdot=48.43299865722656
  AG023.2657+0.0767      Class=HII Region   Mdot=13.26900029182434
  -> 12 with measured inflow; median Mdot=1.22e+01 Msun/yr
Wrote wells_flowrates_byclass.fits