Abstract
We report NH3 observations of the Sgr A complex region including Sgr A West and the 20 km/s and 50 km/s molecular clouds (M-0. 13-0. 08 and M-0.02-0.07) using the Nobeyama Millimeter Array and the 45m telescope. NH3(1,1) and (2,2) lines were simultaneously observed to estimate the kinetic temperature. Our results suggest strong interaction between the molecular clouds and the continuum sources in the Sgr A complex. The interaction with continuum sources might be an important factor in determining the physical conditions of molecular gas in the galactic center region.
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Okumura, S.K. et al. (1989). NH3 Observations of the Sgr A Complex Region with the Nobeyama Millimeter Array. In: Morris, M. (eds) The Center of the Galaxy. International Astronomical Union Union Astronomique Internationale, vol 136. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-2362-1_49
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DOI: https://doi.org/10.1007/978-94-009-2362-1_49
Publisher Name: Springer, Dordrecht
Print ISBN: 978-0-7923-0222-3
Online ISBN: 978-94-009-2362-1
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