Low energy levels of Fe+24 and Fe+25 and calculation of the Kα and Kβ lines by relativistic perturbation

Details Low energy levels of Fe+24 and Fe+25 and calculation of the Kα and Kβ lines by relativistic perturbation Low energy levels of Fe+24 and Fe+25 and calculation of the Kα and Kβ lines by relativistic perturbation

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995cha%26a..19....1z&link_type=ejournal

Chinese Astronomy and Astrophysics, Volume 19, Issue 1, p. 1-6.

Astronomy and Astrophysics

Astrophysics

Elsevier: X-Ray, X-Ray Binaries, Neutron Stars

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