Physical properties of outflows: Comparing CO and H2O based parameters in Class 0 sources
P. Bjerkeli, R. Liseau, B. Nisini, M. Tafalla, P. Bergman, G. Melnick,, G. Rydbeck

TL;DR
This study compares physical outflow parameters derived from CO and H2O tracers in Class 0 sources, finding consistent results within a factor of a few, thus validating the use of different molecular tracers in outflow analysis.
Contribution
It provides a direct comparison of outflow properties derived from CO and H2O, demonstrating their consistency and validating the use of multiple tracers in outflow studies.
Findings
Outflow parameters from CO and H2O are spatially co-located.
Flow widths are comparable when using both tracers.
Momentum rate and luminosity estimates agree within a factor of 4 and 3, respectively.
Abstract
Context. The observed physical properties of outflows from low-mass sources put constraints on possible ejection mechanisms. Historically, these quantities have been derived from CO using ground-based observations. It is thus important to investigate whether parameters such as momentum rate (thrust) and mechanical luminosity (power) are the same when different molecular tracers are used. Aims. We aim at determining the outflow momentum, dynamical time-scale, thrust, energy and power using CO and H2O as tracers of outflow activity. Methods. Within the framework of the WISH key program, three molecular outflows from Class 0 sources have been mapped using the HIFI instrument aboard Herschel. We use these observations together with previously published H2 data to infer the physical properties of the outflows. We compare the physical properties derived here with previous estimates based on…
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Taxonomy
TopicsAstrophysics and Star Formation Studies · Atmospheric Ozone and Climate · Stellar, planetary, and galactic studies
