Level populations for Be-sequence ions in astrophysical plasmas

Details Level populations for Be-sequence ions in astrophysical plasmas Level populations for Be-sequence ions in astrophysical plasmas

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mnras.207..459k&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 207, March 15, 1984, p. 459-463.

Other

50

Atomic Energy Levels, Beryllium, Cosmic Plasma, Electron States, Isoelectronic Sequence, Cosmochemistry, Electron Density (Concentration), Quasars, Seyfert Galaxies, Solar Corona

Scientific paper

Level populations for the 10 n = 2 states of ions in the Be-sequence from C III to Si XI are presented. The results are for two ranges of electron density (Ne = 108 - 1013cm-3 and Ne = 102 - 107cm-3), the former applicable to the solar corona and transition region and the latter to other astrophysical objects such as quasars and Seyfert galaxies.

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