Atomic Data Needs for Modeling Photoionized Plasmas

Simple item page
dc.creatorSavin, Daniel Wolf
dc.date2001-08-03
dc.date.accessioned2026-07-07T01:59:32Z
dc.date.available2026-07-07T01:59:32Z
dc.descriptionMany of the fundamental questions in astrophysics can be addressed using spectroscopic observations of photoionized cosmic plasmas. However, the reliability of the inferred astrophysics depends on the accuracy of the underlying atomic data used to interpret the collected spectra. In this paper, we review some of the most glaring atomic data needs for better understanding photoionized plasmas.
dc.descriptionTo be published in Spectroscopic Challenges of Photoionized Plasmas, ASP Conference Series, Gary Ferland and Daniel Wolf Savin, eds. 7 pages
dc.identifierhttps://arxiv.org/abs/astro-ph/0108058
dc.identifierhttp://arxiv.org/abs/astro-ph/0108058
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3155
dc.subjectAstrophysics
dc.titleAtomic Data Needs for Modeling Photoionized Plasmas
dc.typetext

Files

Collections

arXiv