No CrossRef data available.
Article contents
SiO Emission from the Orion Nebula
Published online by Cambridge University Press: 14 August 2015
Abstract
SiO emission in both a strong maser transition in the first excited vibrational state and in a weaker transition in the ground vibrational state both arise from the same small region in the Kleinmann-Low Nebula in Orion. Within the errors, the source position coincides with that of the infrared source IRc2.
- Type
- Research Article
- Information
- Symposium - International Astronomical Union , Volume 87: Interstellar Molecules , 1980 , pp. 545 - 548
- Copyright
- Copyright © Reidel 1980