No CrossRef data available.
Article contents
The thermal state of molecular clouds in the Galactic center: evidence for non-photon-driven heating
Published online by Cambridge University Press: 22 May 2014
Abstract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
We have used the Atacama Pathfinder Experiment (APEX) 12 m telescope at 218 GHz to observe molecular clouds simultaneously in the JKaKc = 303→202, 322→221, and 321→220 transitions of para-H2CO to determine kinetic temperatures of the dense gas in the central molecular zone of the Galaxy. Gas kinetic temperatures for individual molecular clouds range from 55 to 125 K or even higher. The molecular clouds at high temperatures may be heated by turbulent dissipation and/or cosmic-rays.
- Type
- Contributed Papers
- Information
- Copyright
- Copyright © International Astronomical Union 2014
References
You have
Access