Work

A 3D radiative transfer framework

Year: 2008

Type: article

Abstract: Aims. We present a general method to solve radiative transfer problems including scattering in the continuum as well as in lines in 3D configurations with periodic boundary conditions.

Source: Astronomy and Astrophysics

DOI: 10.1051/0004-6361:200810239

Authors: P. H. Hauschildt, E. Baron

Institutions: Universität Hamburg, Lawrence Berkeley National Laboratory, University of Oklahoma

Language: English

Topic: Stellar, planetary, and galactic studies

Subfield: Astronomy and Astrophysics

Field: Physics and Astronomy

Domain: Physical Sciences

Open Access status: bronze

Funders: National Science Foundation, U.S. Department of Energy, National Aeronautics and Space Administration, National Energy Research Scientific Computing Center, Deutsche Forschungsgemeinschaft, Office of Science

Awards: G139096350, G1398330795, G1643223109, G193590374, G222768804, Collaborative Research: New Standard Stellar Population Models, G2787076192, SPECTROSCOPIC STUDIES OF SNE IA: FINDING THE RIGHT MODEL, RADIATIVE TRANSFER IN 3-D MOVING FLOWS: UNDERSTAND ING STARS, SUPERNOVAE, AND COSMOLOGY, Collaborative research: Three-Dimensional Simulations of Type Ia Supernovae: Constraining Models with Observations, G7337822738, G7572530592, G8099852790, MULTIWAVELENGTH STUDIES OF SUPERNOVAE

OpenAlex ID: W4302199092

FWCI: 0.789

Cites: 6

Cited by: 12

Related to: 10