Astronomy and Astrophysics – Astrophysics
Scientific paper
1999-06-02
Astronomy and Astrophysics
Astrophysics
4 figures
Scientific paper
10.1086/312164
We present observations of the 5$_{1,5}\to4_{2,2}$ transition of water vapor at 325.15 GHz taken with the CSO telescope towards Orion IRc2. The emission is more extended than that of other molecular species such as CH$_3$OH. However, it is much less extended than the emission of water vapor at 183.31 GHz reported by Cernicharo et al (1994). A comparison of the line intensities at 325.15 GHz and 183.31 GHz puts useful constraints on the density and temperature of the emitting regions and allows an estimate of H_2O abundance, x(H_2O), of $\simeq10^{-4}$ in the Plateau and $\simeq10^{-6}-10^{-5}$ in the Ridge.
Benford Dominic J.
Cernicharo Jose
Gonzalez-Alfonso Eduardo
Mehringer David
Pardo Juan Ramon
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