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H76α Emission from the Sgr A 15 km s−1 Cloud
Published online by Cambridge University Press: 23 September 2016
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 Te ~ 7500 K, slightly lower than measurements of Te in Sgr B2. The deduced number of early stars and the infrared luminosity are consistent with a normal IMF in this cloud.
- Type
- The Environment of the SGR A Complex
- Information
- Symposium - International Astronomical Union , Volume 136: The Galactic Center , 1989 , pp. 389 - 391
- Copyright
- Copyright © Kluwer 1989