Benchmark problems for wavelength dependent continuum radiative transfer

dc.creatorIvezic, Z.
dc.creatorGroenewegen, M.
dc.creatorMenshchikov, A.
dc.creatorSzczerba, R.
dc.date1997-05-20
dc.date.accessioned2026-07-25T12:57:39Z
dc.descriptionWhen verifying a sophisticated numerical code, it is a usual practice to compare the results with reliable solutions obtained by other means. This work provides such solutions for the wavelength dependent dust radiative transfer problem. We define a set of benchmark problems in spherical geometry and solve them by three radiative transfer codes which implement different numerical schemes. Results for the dust temperature and emerging spectra agree to better than 0.1%, and can be used as benchmark solutions for the verification of the dust radiative transfer codes.
dc.description4 pages, 2 Postscript figures (included), uses mn.sty. To appear in Monthly Notices of the Royal Astronomical Society
dc.identifierhttps://arxiv.org/abs/astro-ph/9705154
dc.identifierhttp://arxiv.org/abs/astro-ph/9705154
dc.identifier.urihttps://dspace.dare.co.zw/handle/123456789/13261
dc.subjectAstrophysics
dc.titleBenchmark problems for wavelength dependent continuum radiative transfer
dc.typetext

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