Laboratory Measurement and Theoretical Modeling of K‐Shell X‐Ray Lines from Inner‐Shell Excited and Ionized Ions of Oxygen-Reference-Cited by-同舟云学术

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Laboratory Measurement and Theoretical Modeling of K‐Shell X‐Ray Lines from Inner‐Shell Excited and Ionized Ions of Oxygen

Published:2005-07-10 Issue:2 Volume:627 Page:1066-1071
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Gu Ming Feng,Schmidt Mike,Beiersdorfer Peter,Chen Hui,Thorn Daniel B.,Trabert Elmar,Behar Ehud,Kahn Steven M.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/627/i=2/a=1066/pdf

Reference31 articles.

1. Contrasting the Ultraviolet and X‐Ray OviColumn Density Inferred for the Outflow in NGC 5548

2. Behar, E. & Kahn, S. M. 2002, in NASA Laboratory Astrophysics Workshop, ed. F. Salama (Moffett Field: NASA), 23

3. A Long Look at NGC 3783 with theXMM‐NewtonReflection Grating Spectrometer

4. Laboratory X-Ray Astrophysics

5. Flat-field grating spectrometer for high-resolution soft x-ray and extreme ultraviolet measurements on an electron beam ion trap

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