H76α Emission from the Sgr A 15 km s-1 Cloud

J. T. Armstrong,J. M. Jackson,R. T. R. Ho

doi:10.1007/978-94-009-2362-1_52

H76α Emission from the Sgr A 15 km s-1 Cloud

J. T. Armstrong, J. M. Jackson + Show 1 more

https://doi.org/10.1007/978-94-009-2362-1_52

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Publication Date: Jan 1, 1989

Citations: 1

Affiliation: University of Cologne, Massachusetts Institute of Technology, University of California, Berkeley, Harvard University Press

#Normal IMF #Sgr B2 + Show 7 more

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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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