Astronomy and Astrophysics – Astronomy
Scientific paper
May 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mnras.208..147b&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 208, May 1, 1984, p. 147-159. Research supported by the
Astronomy and Astrophysics
Astronomy
40
Atomic Energy Levels, Atomic Spectra, Line Spectra, Manganese, Oscillator Strengths, Ground State, Hyperfine Structure
Scientific paper
The authors present relative oscillator strengths for 58 lines of Mn I for a range of +0.19 > log (gf) > -3.795 in the excitation interval 0 eV < χ < ≡3 eV. The measurements have been made to a relative accuracy of better than 2 per cent using the Oxford furnace technique, with full allowance for hyperfine structure using the data of Booth et al. The relative values have been placed on an absolute scale using published lifetime data, to an accuracy of about 7 per cent for the ground state lines and 3 per cent for the excited state lines.
Blackwell D. E.
Booth Andrew J.
Petford A. D.
Shallis M. J.
No associations
LandOfFree
Measurement of relative oscillator strengths for MN I Transitions from levels in the range chi between 0 eV and 3 eV 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 Measurement of relative oscillator strengths for MN I Transitions from levels in the range chi between 0 eV and 3 eV, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Measurement of relative oscillator strengths for MN I Transitions from levels in the range chi between 0 eV and 3 eV will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1369472