Keywords :
masers - ISM clouds - HII regions
Abstract:We present the results of a search for ammonia maser emission in 119 Galactic high-mass star-forming regions (HMSFRs) known to host 22GHz H_2_O maser emission. Our survey has led to the discovery ofnon-metastable NH3 inversion line masers toward 14 of these sources. This doubles the number of known non-metastable ammonia masers in our Galaxy, including nine new very high-excitation (J, K)=(9,6) maser sources. These maser lines, including NH_3_ (5,4), (6,4), (6,5), (7,6), (8,6), (9,6), (9,8), (10,8), and (11,9), arise from energy levels of 342K, 513K, 465K, 606K, 834K, 1090K, 942K, 1226K, and 1449K above the ground state. Additionally, we tentatively report a new metastable NH_3_ (3,3) maser in G048.49 and an NH_3_ (7,7) maser in
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