![]() ![]() ![]() We identify some of the most extreme molecular gas temperatures detected in the We detect temperature ranging from 210-580\,K. For the cool component weĭetect rotational temperatures ranging from 20-80\,K, and for the hot component Two rotational temperature components to the data. Using these two samples we create full Boltzmann plots for every source and fit The Galactic Center) using the Australia Telescope Compact Array (ATCA), andĪmmonia lines (J,K) = (8,8)-(14,14) using the 100\,m Green Bank Telescope. J,K=(1,1)-(6,6) inversion transitions from SWAG (Survey of Water and Ammonia in We characterize the temperature for 16 regions,Įxtending out to a projected radius of $\sim$450 pc. Hotter than gas in the Galactic disk, but the mechanism responsible for heating The molecular gas in this region is more than an order of magnitude ![]() Pressure, are key factors for characterizing gas energetics, kinematics, andĮvolution. (CMZ), including temperature, density, thermal pressure, and turbulent Physical properties of the Central Molecular Zone Candelaria and 4 other authors Download PDF Abstract: The inner 300-500 pc of the Milky Way has some of the most extreme gasĬonditions in our Galaxy. Download a PDF of the paper titled Widespread Hot Ammonia in the Central Kiloparsec of the Milky Way, by Tierra M. ![]()
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