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  Studies of highly charged iron ions using electron beam ion traps for interpreting astrophysical spectra

Brown, G. V., Beilmann, C., Bernitt, S., Clementson, J., Eberle, S., Epp, S. W., et al. (2013). Studies of highly charged iron ions using electron beam ion traps for interpreting astrophysical spectra. Physica Scripta, Topical issues, T156: 014001. doi:10.1088/0031-8949/2013/T156/014001.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0019-15A7-5 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0028-E40B-1
Genre: Conference Paper

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2021823.pdf (Publisher version), 284KB
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 Creators:
Brown, G. V., Author
Beilmann, C., Author
Bernitt, S., Author
Clementson, J., Author
Eberle, S, Author
Epp, S. W., Author
Graf, A., Author
Hell, N., Author
Kelley, R. L., Author
Kilbourne, C. A., Author
Kubicek, K.1, Author              
Leutenegger, M. A., Author
Mäckel, V., Author
Porter, F. S., Author
Rudolph, J. K., Author
Simon, M. C., Author
Steinbrügge, R., Author
Träbert, E., Author
Ullrich, J., Author
López-Urrutia, J. R. Crespo, Author
Beiersdorfer, P., Author more..
Affiliations:
1Research Group of Structural Dynamics of (Bio)chemical Systems, MPI for biophysical chemistry, Max Planck Society, ou_578564              

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 Abstract: For over a decade, the x-ray astrophysics community has enjoyed a fruitful epoch of discovery largely as a result of the successful launch and operation of the high resolution, high sensitivity spectrometers on board the Chandra, XMM-Newton and Suzaku x-ray observatories. With the launch of the x-ray calorimeter spectrometer on the Astro-H x-ray observatory in 2014, the diagnostic power of high resolution spectroscopy will be extended to some of the hottest, largest and most exotic objects in our Universe. The diagnostic utility of these spectrometers is directly coupled to, and often limited by, our understanding of the x-ray production mechanisms associated with the highly charged ions present in the astrophysical source. To provide reliable benchmarks of theoretical calculations and to address specific problems facing the x-ray astrophysics community, electron beam ion traps have been used in laboratory astrophysics experiments to study the x-ray signatures of highly charged ions. A brief overview of the EBIT-I electron beam ion trap operated at Lawrence Livermore National Laboratory and the Max-Planck-Institut für Kernphysik's FLASH-EBIT operated at third and fourth generation advanced light sources, including a discussion of some of the results are presented.

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Language(s): eng - English
 Dates: 2013-09-232013
 Publication Status: Published in print
 Pages: 3
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 Table of Contents: -
 Rev. Method: Peer
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Title: 16th International Conference on the Physics of Highly Charged Ions
Place of Event: Heidelberg
Start-/End Date: 2012-09-02 - 2012-09-07

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Title: Physica Scripta, Topical issues
Source Genre: Journal
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Pages: - Volume / Issue: T156 Sequence Number: 014001 Start / End Page: - Identifier: ISSN: 0281-1847