De-projection of radio observations of axi-symmetric expanding circumstellar envelopes
P.T. Nhung, D.T. Hoai, P. Tuan-Anh, P. Darriulat, T. Le Bertre, J.M., Winters, P.N. Diep, N.T. Phuong

TL;DR
This paper develops methods for de-projecting radio observations of axi-symmetric expanding circumstellar envelopes, enabling better analysis of their physical properties through effective emissivity and wind velocity modeling.
Contribution
It introduces tools to measure and constrain key parameters of the wind velocity distribution from radio observations, simplifying the analysis process.
Findings
Effective emissivity can be calculated given known wind velocity distribution.
Tools developed help constrain the orientation and shape parameters of the envelope.
Case studies demonstrate practical application with ALMA and NOEMA data.
Abstract
The problem of de-projection of radio line observations of axi-symmetric expanding circumstellar envelopes is studied with the aim of easing their analysis in terms of physics models. The arguments developed rest on the remark that, in principle, when the wind velocity distribution is known, the effective emissivity can be calculated at any point in space. The paper provides a detailed study of how much this is true in practice. The wind velocity distribution assumed to be axi-symmetric and in expansion, is described by four parameters: the angles defining the orientation of the symmetry axis, an overall velocity scale and a parameter measuring the elongation (prolateness) of the distribution. Tools are developed that allow for measuring, or at least constraining, each of the four parameters. The use of effective emissivity as relevant quantity, rather than temperature and density being…
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