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Ammonia Fitting of Multiple Velocity Components in High-Mass Star-Forming Regions
We perform a multiple velocity component analysis of ammonia (NH$_3$) gas from KEYSTONE, a Green Bank Telescope survey covering 11 giant molecular clouds (GMCs) at distances from 0.7 to 2.7 kpc. We extend existing codes to enable simultaneous fitting of up to three velocity components in NH$_3$ (1,1
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