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Improved wavelengths of Fe V and Ni V for analysis of spectra of white dwarf stars

Published online by Cambridge University Press:  18 July 2017

J. Ward  and
G. Nave
J. Ward
Affiliation:
Dept. of Physics, Arizona State University, Tempe, AZ, United States
G. Nave
Affiliation:
National Institute of Standards and Technology, Gaithersburg, MD, USA
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Abstract

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We summarize measurements of improved wavelengths of Fe V and Ni V in the vacuum ultraviolet.

Keywords

atomic data
Type
Addendum
Information
Proceedings of the International Astronomical Union , Volume 11 , General Assembly A29A: Astronomy in Focus , August 2015 , E8
Copyright
Copyright © International Astronomical Union 2017 

References

Berengut, J. C., Flambaum, V. V., Ong, A., Webb, J. K., Barrow, J. D., Barstow, M. A., Preval, S. P., & Holberg, J. B. 2013, Phys. Rev. Lett. 111, 010801 CrossRefGoogle Scholar