Abstract
We present Infrared Space Observatory (ISO) observations of 16OH and 18OH toward Sgr B2 with a spectral resolution of ~35 km s-1. The OH J=5/2-->3/2 and J=3/2-->1/2 rotational lines of the 2Π1/2 ladder are seen in emission, while the cross-ladder transitions (from the 2Π3/2 J=3/2 to the J=1/2, 3/2, and 5/2 levels of the 2Π1/2 ladder) and the 2Π3/2 J=5/2
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CITATION STYLE
APA
Goicoechea, J. R., & Cernicharo, J. (2002). Far-Infrared OH Fluorescent Emission in Sagittarius B2. The Astrophysical Journal, 576(1), L77–L81. https://doi.org/10.1086/343062
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