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Ray Tracing for Complex Astrophysical High‐opacity Structures

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Outgoing claims: the papers this work cites, builds on, or argues with.

inferredcites →https://doi.org/10.1016/0022-4073(96)00053-2openalex-snapshot
Efficient integration of intensity functions on the unit sphere
inferredcites →https://doi.org/10.1016/j.newast.2005.09.004openalex-snapshot
C2-ray: A new method for photon-conserving transport of ionizing radiation
inferredcites →https://doi.org/10.1016/s0010-4655(02)00675-6openalex-snapshot
MC3D–3D continuum radiative transfer, Version 2
inferredcites →https://doi.org/10.1016/s0022-4073(01)00195-9openalex-snapshot
Radiative transfer through a spherically symmetric cloud of extincting particles — exact solution of the inverse absorption problem
inferredcites →https://doi.org/10.1016/s0022-4073(02)00042-0openalex-snapshot
Application of adaptive multi-frequency grids to three-dimensional astrophysical radiative transfer
inferredcites →https://doi.org/10.1051/0004-6361:20010778openalex-snapshot
The dust temperature distribution in prestellar cores
inferredcites →https://doi.org/10.1051/0004-6361:20010778/pdfopenalex-snapshot
The dust temperature distribution in prestellar cores
inferredcites →https://doi.org/10.1051/0004-6361:20021853openalex-snapshot
3D continuum radiative transfer in complex dust configurations around stellar objects and active galactic nuclei
inferredcites →https://doi.org/10.1051/0004-6361:20040017openalex-snapshot
The 2D continuum radiative transfer problem
inferredcites →https://doi.org/10.1051/0004-6361:20041978openalex-snapshot
3D continuum radiative transfer in complex dust configurations
inferredcites →https://doi.org/10.1086/162480openalex-snapshot
Optical properties of interstellar graphite and silicate grains
inferredcites →https://doi.org/10.1086/309198openalex-snapshot
Photoevaporation of Protostellar Disks. V. Circumstellar Disks under the Influence of Both Extreme‐Ultraviolet and Far‐Ultraviolet Radiation
inferredcites →https://doi.org/10.1086/339264openalex-snapshot
On the Formation of Massive Stars
inferredcites →https://doi.org/10.1086/426053openalex-snapshot
Three-dimensional Continuum Radiative Transfer Images of a Molecular Cloud Core Evolution
inferredcites →https://doi.org/10.1086/426111openalex-snapshot
Obscuration of Active Galactic Nuclei by Circumnuclear Starbursts
inferredcites →https://doi.org/10.1086/432614openalex-snapshot
The Discovery of a Massive SCUBA Core with both Inflow and Outflow Motions
inferredcites →https://doi.org/10.1145/79505.79507openalex-snapshot
A variable order Runge-Kutta method for initial value problems with rapidly varying right-hand sides
inferredcites →https://doi.org/10.1146/annurev.aa.28.090190.001511openalex-snapshot
Quantitative Spectroscopy of Hot Stars

What points at this work

Incoming claims: where this work appears in other papers’ reference lists and arguments.

inferred← citeshttps://doi.org/10.2139/ssrn.4873795openalex-extracted
Quasi-Monte Carlo Radiative Transfer
inferred← citeshttps://doi.org/10.1007/978-3-642-03370-4_4openalex-snapshot
Three Dimensional Continuum Radiative Transfer
inferred← citeshttps://doi.org/10.1016/j.ascom.2018.06.002openalex-snapshot
Three-dimensional heuristic radiation transfer method based on enumeration using the directions grid
inferred← citeshttps://doi.org/10.1017/s1743921311000779openalex-snapshot
Radiative Transfer Modeling of Simulation and Observational Data
inferred← citeshttps://doi.org/10.1051/0004-6361/200912437openalex-snapshot
Comparing the statistics of interstellar turbulence in simulations and observations
inferred← citeshttps://doi.org/10.1051/0004-6361/201014511openalex-snapshot
Fast ray-tracing algorithm for circumstellar structures (FRACS) I. Algorithm description and parameter-space study for mid-IR interferometry of B[e] stars
inferred← citeshttps://doi.org/10.1051/0004-6361/201014669openalex-snapshot
The structured environments of embedded star-forming cores
inferred← citeshttps://doi.org/10.1051/0004-6361/201015217openalex-snapshot
Modelling the spectral energy distribution of galaxies
inferred← citeshttps://doi.org/10.1051/0004-6361/201117150openalex-snapshot
HYPERION: an open-source parallelized three-dimensional dust continuum radiative transfer code
inferred← citeshttps://doi.org/10.1051/0004-6361/201322281openalex-snapshot
Using 3D Voronoi grids in radiative transfer simulations
inferred← citeshttps://doi.org/10.1051/0004-6361/201322281/pdfopenalex-snapshot
Using 3D Voronoi grids in radiative transfer simulations
inferred← citeshttps://doi.org/10.1051/0004-6361/201322593openalex-snapshot
Hierarchical octree andk-d tree grids for 3D radiative transfer simulations
inferred← citeshttps://doi.org/10.1051/0004-6361/201424930openalex-snapshot
Radiative transfer with POLARIS
inferred← citeshttps://doi.org/10.1051/eas/0935015openalex-snapshot
Radiative transfer modeling of complex dusty structures
inferred← citeshttps://doi.org/10.1086/529364openalex-snapshot
Modeling the Dust Properties ofz∼ 6 Quasars with ART2—All‐Wavelength Radiative Transfer with Adaptive Refinement Tree
inferred← citeshttps://doi.org/10.1109/rose52750.2021.9611767openalex-snapshot
Ray Tracing 3D Source Modelling for Optical Reflectance Sensing with Wireless Ranging Application
inferred← citeshttps://doi.org/10.1111/j.1365-2966.2008.14316.xopenalex-snapshot
Effects of scattering and dust grain size on the temperature structure of protoplanetary discs: a three-layer approach
inferred← citeshttps://doi.org/10.1111/j.1365-2966.2012.21228.xopenalex-snapshot
ART2: coupling Lyα line and multi-wavelength continuum radiative transfer
inferred← citeshttps://doi.org/10.1134/s1063773719100062openalex-snapshot
Influence of Large-Scale Perturbations in Circumstellar Disks on the Linear Polarization Parameters of UX Ori Stars
inferred← citeshttps://doi.org/10.1137/090764542openalex-snapshot
Diffusive Corrections to $P_N$ Approximations
inferred← citeshttps://doi.org/10.1146/annurev-astro-082812-141042openalex-snapshot
Three-Dimensional Dust Radiative Transfer
inferred← citeshttps://doi.org/10.48550/arxiv.0905.1060openalex-snapshot
Comparing the statistics of interstellar turbulence in simulations and observations: Solenoidal versus compressive turbulence forcing
inferred← citeshttps://doi.org/10.48550/arxiv.1011.2942openalex-snapshot
Modelling the spectral energy distribution of galaxies. V. The dust and PAH emission SEDs of disk galaxies
inferred← citeshttps://doi.org/10.48550/arxiv.1604.05305openalex-snapshot
Radiative transfer with POLARIS: I. Analysis of magnetic fields through synthetic dust continuum polarization measurements
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