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New interstellar masers in nonmetastable ammonia

Journal Article · · Astrophys. J., Lett. Ed.; (United States)
DOI:https://doi.org/10.1086/184607· OSTI ID:6060198
We report the first astronomical detections of several ammonia inversion transitions involving nonmetastable levels with energies as high as 1090 K above the ground state. The (J,K) = (9,6) inversion transition shows maser-like emission in the directions of W51,NGC 7538, W49, and DR 21(OH). The NH/sub 3/ (6,3) line exhibits similar characteristics in W51 but is seen in absorption in NGC 7538. These are the first definite detections of ammonia masers in space. The intensities and narrow line widths (0.5--1.5 km s/sup -1/) for the emission features are in contrast to the previously detected broad, weak, nonmetastable lines attributed to thermal emission in these sources. Temporal variability appears to be evident in the (9,6) emission in W49 over a 4 month period. The highly excited (J,K) = (9,6) and (6,3) ammonia lines are found in regions containing compact H II regions and strong infrared sources with associated H/sub 2/O and OH masers; i.e., in regions of active star formation.
Research Organization:
Department of Physics and Astronomy and Five College Radio Astronomy Observatory, University of Massachusetts
OSTI ID:
6060198
Journal Information:
Astrophys. J., Lett. Ed.; (United States), Journal Name: Astrophys. J., Lett. Ed.; (United States) Vol. 300:2; ISSN AJLEA
Country of Publication:
United States
Language:
English