Young T Tauri star in CB 26 molecular outflows (Launhardt+, 2009)

Physics

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Molecular Clouds, Stars: Pre-Main Sequence

Scientific paper

The IRAM PdBI array was used to observe 12CO(2-1) at 1.3mm configurations, resulting in spectral line maps with 1.5" resolution. We use an empirical parameterized steady-state outflow model combined with 2-D line radiative transfer calculations and chi2-minimization in parameter space to derive a best-fit model and constrain parameters of the outflow.
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