Auger decay of light cosmic ions - Overwhelming population of final excited states

Details Auger decay of light cosmic ions - Overwhelming population of final excited states Auger decay of light cosmic ions - Overwhelming population of final excited states

Nov 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...265..857p&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 265, no. 2, p. 857, 858.

Astronomy and Astrophysics

Astrophysics

1

Cosmic Plasma, Decay, Interstellar Matter, Light Ions, Molecular Excitation, Photoionization, Active Galactic Nuclei, Neon

Scientific paper

A previous work (Petrini and Tully, 1991) presented a particular feature of the Auger process following K-ionization of atomic B-like ions or 1s-2p excitation of Be-like ions, i.e., the overwhelming population of 2p excited final state. It was noted in that work that this selective production also concerns most of the 1s-hole states of light ions. In the present paper, this statement is confirmed after analysis of the Auger decay of Ne ions, with Ne(4+) chosen as an example of a light cosmic ion.

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