NIII and NIV line emission following K-shell photoionization.

Details NIII and NIV line emission following K-shell photoionization. NIII and NIV line emission following K-shell photoionization.

Oct 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997a%26a...326..870p&link_type=abstract

Astronomy and Astrophysics, v.326, p.870-872

Astronomy and Astrophysics

Astrophysics

1

Atomic Processes, Atomic Data, Uv: General, X-Rays: General

Scientific paper

Soft X-ray irradiation of low density cold matter K-ionizes neutral
nitrogen. The full ionization process followed by Auger decay populates
the excited states of NIII and NIV ions. NIII and NIV uv lines are
therefore produced directly with comparable intensities. Some observable
intensity ratios are evaluated.

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