X-ray emission line profile modeling of hot stars

Roban H. Kramer, Stephanie K. Tonnesen, David H. Cohen, Stanley P. Owocki, Asif Ud-Doula, Joseph J. MacFarlane

Research output: Contribution to journalConference article

3 Scopus citations

Abstract

A study was performed on x-ray emission line profile modeling of hot stars. The quantitative models of both a spherically symmetric wind and a wind with hot plasma confined in an equatorial disk by a dipole magnetic field were discussed. It was found that the emergent line profiles were affected by transport through a two-component, moving, optically thick medium.

Original languageEnglish (US)
Pages (from-to)1966-1968
Number of pages3
JournalReview of Scientific Instruments
Volume74
Issue number3 II
DOIs
StatePublished - Mar 2003
EventProceedings of the 14th Topical Conference on High - Temperature Plasma Diagnostics - Madison, WI, United States
Duration: Jul 8 2002Jul 11 2002

All Science Journal Classification (ASJC) codes

  • Instrumentation

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    Kramer, R. H., Tonnesen, S. K., Cohen, D. H., Owocki, S. P., Ud-Doula, A., & MacFarlane, J. J. (2003). X-ray emission line profile modeling of hot stars. Review of Scientific Instruments, 74(3 II), 1966-1968. https://doi.org/10.1063/1.1535240