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• W3100244695 endingPage "105" @default.
• W3100244695 startingPage "105" @default.
• W3100244695 abstract "We present the detection of metastable inversion lines of ammonia from energy levels high above the ground state. We detect these lines in both emission and absorption toward fifteen of seventeen positions in the central 300 parsecs of the Galaxy. In total, we observe seven metastable transitions of ammonia: (8,8), (9,9), (10,10), (11,11), (12,12), (13,13) and (15,15), with energies (in Kelvins) ranging from 680 to 2200 K. We also map emission from ammonia (8,8) and (9,9) in two clouds in the Sgr A complex (M-0.02-0.07 and M-0.13-0.08), and we find that the line emission is concentrated toward the the dense centers of these molecular clouds. The rotational temperatures derived from the metastable lines toward M-0.02-0.07 and M-0.13-0.08 and an additional cloud (M0.25+0.01) range from 350 to 450 K. Similarly highly-excited lines of ammonia have previously been observed toward Sgr B2, where gas with kinetic temperatures of ~600 K has been inferred. Our observations show that the existence of a hot molecular gas component is not unique to Sgr B2, but rather appears common to many Galactic center molecular clouds. In M-0.02-0.07, we find that the hot ammonia, contributes ~10% of the cloud's total ammonia column density, and further, that the hot ammonia in this cloud arises in gas which is extended or uniformly distributed on ~10 arcsecond scales. We discuss the implications of these constraints upon the nature of this hot gas component. In addition to the detection of hot metastable ammonia line emission, we also detect for the first time emission from nonmetastable inversion transitions of ammonia in both M-0.02-0.07 and M-0.13-0.08." @default.
• W3100244695 created "2020-11-23" @default.
• W3100244695 creator A5058769617 @default.
• W3100244695 creator A5059319698 @default.
• W3100244695 date "2013-07-11" @default.
• W3100244695 modified "2023-10-12" @default.
• W3100244695 title "DETECTION OF WIDESPREAD HOT AMMONIA IN THE GALACTIC CENTER" @default.
• W3100244695 cites W1487272948 @default.
• W3100244695 cites W1965545286 @default.
• W3100244695 cites W1968685979 @default.
• W3100244695 cites W1973813727 @default.
• W3100244695 cites W1975803861 @default.
• W3100244695 cites W1977152037 @default.
• W3100244695 cites W1978782810 @default.
• W3100244695 cites W1979081980 @default.
• W3100244695 cites W1979765307 @default.
• W3100244695 cites W1984922085 @default.
• W3100244695 cites W1989706846 @default.
• W3100244695 cites W1998270955 @default.
• W3100244695 cites W1998936450 @default.
• W3100244695 cites W2000032841 @default.
• W3100244695 cites W2002280578 @default.
• W3100244695 cites W2004519051 @default.
• W3100244695 cites W2005751044 @default.
• W3100244695 cites W2011491298 @default.
• W3100244695 cites W2013535230 @default.
• W3100244695 cites W2022787705 @default.
• W3100244695 cites W2024525569 @default.
• W3100244695 cites W2026552946 @default.
• W3100244695 cites W2031070315 @default.
• W3100244695 cites W2032202691 @default.
• W3100244695 cites W2035088604 @default.
• W3100244695 cites W2035878314 @default.
• W3100244695 cites W2039741247 @default.
• W3100244695 cites W2041136900 @default.
• W3100244695 cites W2041936494 @default.
• W3100244695 cites W2049871984 @default.
• W3100244695 cites W2054316599 @default.
• W3100244695 cites W2054498796 @default.
• W3100244695 cites W2061828051 @default.
• W3100244695 cites W2065733335 @default.
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• W3100244695 cites W2086140797 @default.
• W3100244695 cites W2088754872 @default.
• W3100244695 cites W2092456387 @default.
• W3100244695 cites W2105443995 @default.
• W3100244695 cites W2114773466 @default.
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• W3100244695 cites W2339190438 @default.
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• W3100244695 cites W3098272548 @default.
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• W3100244695 cites W3100093506 @default.
• W3100244695 cites W3101778427 @default.
• W3100244695 cites W3104142665 @default.
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• W3100244695 cites W3104712426 @default.
• W3100244695 cites W3106020236 @default.
• W3100244695 cites W3121726213 @default.
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• W3100244695 cites W4291818096 @default.
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• W3100244695 doi "https://doi.org/10.1088/0004-637x/772/2/105" @default.
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