2023ApJ...946...23L


Query : 2023ApJ...946...23L

2023ApJ...946...23L - Astrophys. J., 946, 23 (2023/March-3)

Emission Lines of Fe XIV, Fe XV, and Fe XVI in the Extreme Ultraviolet Region 40-100 Å.

LEPSON J.K., BEIERSDORFER P., BROWN G.V. and LIEDAHL D.A.

Abstract (from CDS):

We report on emission spectra of iron in the extreme ultraviolet recorded at an electron density of ∼1011 cm–3 on the Lawrence Livermore electron beam ion trap facility. We present a summary of the observed emission lines, including wavelengths and emission intensities, and present spectra of pure Fe XIV through Fe XVI emission derived from our measurements in the 40-100 Å wavelength range. We show that spectral models, especially the current version of CHIANTI v10.0, describe the M-shell emission from these three charge states of iron reasonably well, and we are able to verify several transitions in CHIANTI for the first time.

Abstract Copyright: © 2023. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Stellar coronae - Laboratory astrophysics - Atomic spectroscopy - Line positions

Simbad objects: 4

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Number of rows : 4
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
#notes
1 * alf CMi SB* 07 39 18.11950 +05 13 29.9552 0.82 0.79 0.37 -0.05 -0.28 F5IV-V+DQZ 1872 0
2 * alf Cen ** 14 39 36.50 -60 50 02.3   0.4 -0.1     G2V+K1V 961 0
3 * i Boo ** 15 03 47.29565 +47 39 14.6228           G0Vn 546 0
4 HD 197481 BY* 20 45 09.5324974119 -31 20 27.237889841   10.05 8.627 9.078 6.593 M1VeBa1 1174 0

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