Synthetic Spectrum Methods for Three-Dimensional Supernova Models

Simple item page
dc.creatorThomas, R. C.
dc.date2003-10-21
dc.date.accessioned2026-07-07T02:10:44Z
dc.date.available2026-07-07T02:10:44Z
dc.descriptionCurrent observations stimulate the production of fully three-dimensional explosion models, which in turn motivates three-dimensional spectrum synthesis for supernova atmospheres. We briefly discuss techniques adapted to address the latter problem, and consider some fundamentals of line formation in supernovae without recourse to spherical symmetry. Direct and detailed extensions of the technique are discussed, and future work is outlined.
dc.description6 pages, 3 figures, to appear in proc. "3-D Signatures in Stellar Explosions", Austin, Texas
dc.identifierhttps://arxiv.org/abs/astro-ph/0310619
dc.identifierhttp://arxiv.org/abs/astro-ph/0310619
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6834
dc.subjectAstrophysics
dc.titleSynthetic Spectrum Methods for Three-Dimensional Supernova Models
dc.typetext

Files

Collections

arXiv