On the influence of collisional rate coefficients on the water vapour excitation
F. Daniel, J. R. Goicoechea, J. Cernicharo, M.-L. Dubernet, A. Faure

TL;DR
This study evaluates how different collisional rate coefficients affect water vapor excitation modeling in astrophysical environments, revealing potential inaccuracies in abundance estimates when using certain CRC sets under specific conditions.
Contribution
It provides a detailed comparison of CRC sets for H$_2$O, highlighting the impact on line intensity predictions and abundance estimates in astrophysical models.
Findings
Quantum and QCT CRCs agree well at high densities.
Differences up to a factor of 3 in line intensities at low densities.
Using QCT CRCs can lead to underestimation of water abundance.
Abstract
Water is a key molecule in many astrophysical studies. Its high dipole moment makes this molecule to be subthermally populated under the typical conditions of most astrophysical objects. This motivated the calculation of various sets of collisional rate coefficients (CRC) for HO (with He or H) which are necessary to model its rotational excitation and line emission. We performed accurate non--local non--LTE radiative transfer calculations using different sets of CRC in order to predict the line intensities from transitions that involve the lowest energy levels of HO (E 900 K). The results obtained from the different CRC sets are then compared using line intensity ratio statistics. For the whole range of physical conditions considered in this work, we obtain that the intensities based on the quantum and QCT CRC are in good agreement. However, at relatively low H…
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