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Observation of Diffuse CII Emission in the Galactic Center Region
Published online by Cambridge University Press: 23 September 2016
Abstract
Spectroscopic observations of CII line emission at 157.7 μm have been made of the Galactic Center region with a Fabry-Perot spectrometer onboard a balloon telescope. Strong emission has been detected ubiquitously in a wide area extending between ± 0.7° in galactic longitude. A ring-like structure is suggested from the double lobed distribution of the emission around the Galactic Center.
- Type
- The Large - Scale Interstellar Medium
- Information
- Symposium - International Astronomical Union , Volume 136: The Galactic Center , 1989 , pp. 145 - 149
- Copyright
- Copyright © Kluwer 1989