Plasma environment effects on K lines of astrophysical interest: II. Ionization potentials, K thresholds, radiative rates, and Auger widths in Ne-Through He-like iron ions (Feâ XVII-Feâ XXV)

被引：0

作者：

Deprince, J. ^{[1
]}

Bautista, M.A. ^{[2
]}

Fritzsche, S. ^{[3
,4
]}

García, J.A. ^{[5
,6
]}

Kallman, T. ^{[7
]}

Mendoza, C. ^{[2
]}

Palmeri, P. ^{[1
]}

Quinet, P. ^{[1
,8
]}

机构：

[1] Physique Atomique et Astrophysique, Université de Mons UMONS, Mons,7000, Belgium

[2] Department of Physics, Western Michigan University, Kalamazoo,MI,49008, United States

[3] Helmholtz Institut Jena, Jena,07743, Germany

[4] Theoretisch Physikalisches Institut, Friedrich Schiller Universität Jena, Jena,07743, Germany

[5] Cahill Center for Astronomy and Astrophysics, California Institute of Technology, Pasadena,CA,91125, United States

[6] Dr. Karl Remeis-Observatory and Erlangen Centre for Astroparticle Physics, Sternwartstr. 7, Bamberg,96049, Germany

[7] NASA Goddard Space Flight Center, Greenbelt,MD,662, United States

[8] IPNAS, Université de Liège, Sart Tilman 4000, Liège, Belgium

来源：

Astronomy and Astrophysics | 2019年 / 626卷

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