Laboratory Data on the EUV/Soft-X-Ray Flux Problem of Fe xviii and Fe xix | Zendy

E. Träbert | Zendy; P. Beiersdörfer | Zendy

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Laboratory Data on the EUV/Soft-X-Ray Flux Problem of Fe xviii and Fe xix

Author(s) -

E. Träbert,

P. Beiersdörfer

Publication year - 2021

Publication title -

the astrophysical journal

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 2.376

H-Index - 489

eISSN - 1538-4357

pISSN - 0004-637X

DOI - 10.3847/1538-4357/abef66

Subject(s) - physics , astrophysics , extreme ultraviolet , flux (metallurgy) , spectrometer , emission spectrum , extreme ultraviolet lithography , line (geometry) , electron beam ion trap , spectral line , astronomy , interstellar medium , electron , cathode ray , optics , galaxy , laser , materials science , geometry , mathematics , metallurgy , quantum mechanics

Observations by the spacecraft Extreme Ultraviolet Explorer (EUVE), Far Ultraviolet Spectroscopic Explorer (FUSE), Chandra, and XMM-Newton of Capella ( α Aurigae) have encountered problems with the relative intensities of the Fe xviii and Fe xix line emission in the soft-X-ray (XUV) and extreme-ultraviolet spectral ranges versus various model predictions based on theoretical atomic data. The reason may either lie in astrophysical phenomena, e.g., at emission or because of absorption by the interstellar medium, in the theoretical atomic data, in one or more spectrometer calibrations, or in the spectral modeling. By measurements using an electron beam ion trap we provide laboratory data obtained under conditions that are reasonably close to stellar emission regions. The laboratory data on Fe xviii and Fe xix show line ratios that are rather similar to the observations of Capella. The measurements, therefore, rule out astrophysical phenomena and calibration errors and point to issues with the modeling of the observed Capella emission.

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