Abstract
We report VLA observations of H76α emission from the H II region in M-0.13-0.08, the Sgr A “15 km s-1 cloud.” The line to continuum flux ratio implies an electron temperature T e ~ 7500 K, slightly lower than measurements of T e in Sgr B2. The deduced number of early stars and the infrared luminosity are consistent with a normal IMF in this cloud.
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Armstrong, J.T., Jackson, J.M., Ho, R.T.R. (1989). H76α Emission from the Sgr A 15 km s-1 Cloud. 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_52
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DOI: https://doi.org/10.1007/978-94-009-2362-1_52
Publisher Name: Springer, Dordrecht
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