Herschel observations of Extra-Ordinary Sources: Methanol as a probe of physical conditions in Orion KL
S. Wang, E. A. Bergin, N. R. Crockett, P. F. Goldsmith, D. C. Lis, J., C. Pearson, P. Schilke, T. A. Bell, C. Comito, G.A. Blake, E. Caux, C., Ceccarelli, J. Cernicharo, F. Daniel, M.-L. Dubernet, M. Emprechtinger, P., Encrenaz, M. Gerin, T. F. Giesen, J. R. Goicoechea, H. Gupta

TL;DR
This study uses Herschel/HIFI observations of methanol emission in Orion KL to probe the physical conditions and thermal structure of different spatial components, revealing external heating of the compact ridge.
Contribution
First detailed analysis of methanol emission lines in Orion KL with Herschel, demonstrating their effectiveness in probing physical conditions and thermal structure.
Findings
Methanol lines reveal distinct physical conditions in Orion KL components.
The compact ridge is externally heated, as shown by methanol emission analysis.
Methanol transitions cover a broad energy range, enabling thermal structure mapping.
Abstract
We have examined methanol emission from Orion KL with of the {\em Herschel}/HIFI instrument, and detected two methanol bands centered at 524 GHz and 1061 GHz. The 524 GHz methanol band (observed in HIFI band 1a) is dominated by the isolated J0, K-3, v0 Q branch, and includes 25 E-type and 2 A-type transitions. The 1061 GHz methanol band (observed in HIFI band 4b) is dominated by the J0, K6, v0 Q branch transitions which are mostly blended. We have used the isolated E-type v0 methanol transitions to explore the physical conditions in the molecular gas. With HIFI's high velocity resolution, the methanol emission contributed by different spatial components along the line of sight toward Orion KL (hot core, low velocity flow, and compact ridge) can be distinguished and studied separately. The isolated transitions…
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