Visualisation in Astrophysics

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dc.contributor.authorErtl, T.en_US
dc.contributor.authorGeyer, F.en_US
dc.contributor.authorHerold, H.en_US
dc.contributor.authorKraus, U.en_US
dc.contributor.authorNiemeier, R.en_US
dc.contributor.authorNollert, H.- P.en_US
dc.contributor.authorRebetzky, A.en_US
dc.contributor.authorRuder, H.en_US
dc.contributor.authorZeller, G.en_US
dc.date.accessioned2015-10-05T07:56:08Z
dc.date.available2015-10-05T07:56:08Z
dc.date.issued1989en_US
dc.description.abstractThis paper reports on progress we have made in modelling cosmic X-ray sources on supercomputers. The results we present are meant to serve as an example for the fact that sophisticated visualization techniques play a crucial role in scientific computing. Among the graphical methods we demonstrate, raytracing in curved space-time and a physically motivated 3D-volume rendering algorithm might be of interest to the graphics community in general.en_US
dc.description.seriesinformationEG 1989-Technical Papersen_US
dc.identifier.doi10.2312/egtp.19891011en_US
dc.identifier.issn1017-4656en_US
dc.identifier.urihttps://doi.org/10.2312/egtp.19891011en_US
dc.publisherEurographics Associationen_US
dc.titleVisualisation in Astrophysicsen_US
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EG1989 Proceedings (Technical Papers)