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

doi:10.1063/1.1535240

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

Penn State Scranton

Research output: Contribution to journal › Conference article › peer-review

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 language	English (US)
Pages (from-to)	1966-1968
Number of pages	3
Journal	Review of Scientific Instruments
Volume	74
Issue number	3 II
DOIs	https://doi.org/10.1063/1.1535240
State	Published - Mar 2003
Event	Proceedings of the 14th Topical Conference on High - Temperature Plasma Diagnostics - Madison, WI, United States Duration: Jul 8 2002 → Jul 11 2002

All Science Journal Classification (ASJC) codes

Instrumentation

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10.1063/1.1535240

Cite this

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title = "X-ray emission line profile modeling of hot stars",

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.",

author = "Kramer, \{Roban H.\} and Tonnesen, \{Stephanie K.\} and Cohen, \{David H.\} and Owocki, \{Stanley P.\} and Asif Ud-Doula and MacFarlane, \{Joseph J.\}",

year = "2003",

month = mar,

doi = "10.1063/1.1535240",

language = "English (US)",

volume = "74",

pages = "1966--1968",

journal = "Review of Scientific Instruments",

issn = "0034-6748",

publisher = "American Institute of Physics",

number = "3 II",

note = "Proceedings of the 14th Topical Conference on High - Temperature Plasma Diagnostics ; Conference date: 08-07-2002 Through 11-07-2002",

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TY - JOUR

T1 - X-ray emission line profile modeling of hot stars

AU - Kramer, Roban H.

AU - Tonnesen, Stephanie K.

AU - Cohen, David H.

AU - Owocki, Stanley P.

AU - Ud-Doula, Asif

AU - MacFarlane, Joseph J.

PY - 2003/3

Y1 - 2003/3

N2 - 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.

AB - 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.

UR - https://www.scopus.com/pages/publications/0037348228

UR - https://www.scopus.com/pages/publications/0037348228#tab=citedBy

U2 - 10.1063/1.1535240

DO - 10.1063/1.1535240

M3 - Conference article

AN - SCOPUS:0037348228

SN - 0034-6748

VL - 74

SP - 1966

EP - 1968

JO - Review of Scientific Instruments

JF - Review of Scientific Instruments

IS - 3 II

T2 - Proceedings of the 14th Topical Conference on High - Temperature Plasma Diagnostics

Y2 - 8 July 2002 through 11 July 2002

ER -

X-ray emission line profile modeling of hot stars

Abstract

All Science Journal Classification (ASJC) codes

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