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Three-Dimensional Radiative TransferRadiative Transfer (RT) effects play a crucial role in the thermal history of the intergalactic medium. Here I discuss recent advances in the development of numerical methods that introduce RT to cosmological hydrodynamics. These methods can also readily be applied to time dependent problems on interstellar and galactic scales.
Document ID
20000090663
Acquisition Source
Goddard Space Flight Center
Document Type
Conference Paper
Authors
Abel, Tom (Harvard-Smithsonian Center for Astrophysics Cambridge, MA United States)
Date Acquired
August 19, 2013
Publication Date
May 1, 2000
Publication Information
Publication: Astrophysical Plasmas: Codes, Models, and Observations
Volume: 9
Subject Category
Astrophysics
Funding Number(s)
CONTRACT_GRANT: NAG5-4236
CONTRACT_GRANT: NAG5-3923
Distribution Limits
Public
Copyright
Other

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