Autoionized levels and oscillator strengths for SiII

Details Autoionized levels and oscillator strengths for SiII Autoionized levels and oscillator strengths for SiII

May 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26as...44..171a&link_type=abstract

Astronomy and Astrophysics Supplement Series, vol. 44, May 1981, p. 171-178.

Astronomy and Astrophysics

Astrophysics

45

A Stars, Atomic Energy Levels, Autoionization, Magnetic Stars, Silicon, Transition Probabilities, Atomic Structure, Line Spectra, Tables (Data)

Scientific paper

The strong absorption around 1400 A which appears in Si magnetic Ap stars has been attributed to the autoionization lines of Si II. In order to verify this, the atomic structure of Si II was computed to obtain characteristics of lines connecting discrete excited and quasi-discrete broadened levels. Seventy-one Si II terms were calculated between the first Si(plus) limit and 200,000 per cm. The widths of the terms which are broadened by autoionization effects are given down to 0.000001 eV. A list of 809 lines of Si II in the range 900-8000 A was compiled, and the oscillator strengths were calculated.

Affiliated with

Also associated with

No associations

Rating

Autoionized levels and oscillator strengths for SiII does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Autoionized levels and oscillator strengths for SiII, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Autoionized levels and oscillator strengths for SiII will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1440750