AVIATOR: Morphological object reconstruction in 3D. An application to dense cores
arXiv:1912.01005 · doi:10.1051/0004-6361/201936095
Abstract
Reconstructing 3D distributions from their 2D projections is a ubiquitous problem in various scientific fields, particularly so in observational astronomy. In this work, we present a new approach to solving this problem: a Vienna inverse-Abel-transform based object reconstruction algorithm AVIATOR. The reconstruction that it performs is based on the assumption that the distribution along the line of sight is similar to the distribution in the plane of projection, which requires a morphological analysis of the structures in the projected image. The output of the AVIATOR algorithm is an estimate of the 3D distribution in the form of a reconstruction volume that is calculated without the problematic requirements that commonly occur in other reconstruction methods such as symmetry in the plane of projection or modelling of radial profiles. We demonstrate the robustness of the technique to different geometries, density profiles, and noise by applying the AVIATOR algorithm to several model objects. In addition, the algorithm is applied to real data: We reconstruct the density and temperature distributions of two dense molecular cloud cores and find that they are in excellent agreement with profiles reported in the literature. The AVIATOR algorithm is thus capable of reconstructing 3D distributions of physical quantities consistently using an intuitive set of assumptions.
11 pages, 16 figures, accepted for publication by Astronomy & Astrophysics. v2: Typo in Eq. 3 corrected. The AVIATOR code and a Jupyter notebook illustrating its use is publicly available at https://github.com/BirgitHa/AVIATOR
References in corpus (9)
- The NumPy array: a structure for efficient numerical computation
- scikit-image: Image processing in Python
- Herschel-Planck dust optical-depth and column-density maps: I. Method description and results for Orion
- Unfolding the Laws of Star Formation: The Density Distribution of Molecular Clouds
- A direct comparison of high-speed methods for the numerical Abel transform
- The Earliest Phases of Star formation observed with Herschel (EPoS): The dust temperature and density distributions of B68
- Probing changes of dust properties along a chain of solar-type prestellar and protostellar cores in Taurus with NIKA
- HP2 survey: III The California Molecular Cloud--A Sleeping Giant Revisited
- Prestellar core modeling in the presence of a filament - The dense heart of L1689B