Transition probabilities and lifetimes in neutral and singly ionized osmium and the Solar osmium abundance

Details Transition probabilities and lifetimes in neutral and singly ionized osmium and the Solar osmium abundance Transition probabilities and lifetimes in neutral and singly ionized osmium and the Solar osmium abundance

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006a%26a...448.1207q&link_type=abstract

Astronomy and Astrophysics, Volume 448, Issue 3, March IV 2006, pp.1207-1216

Astronomy and Astrophysics

Astrophysics

16

Sun: Abundances, Atomic Data, Atomic Processes

Scientific paper

Radiative lifetime measurements have been performed, with a time-resolved laser-induced fluorescence technique, for 12 levels of Os I and for 9 levels of Os II. For 9 levels of Os I and 4 levels of Os II, there were no previous experimental data available. From a comparison with new theoretical calculations, taking configuration interactions and core-polarization effects into account, it has been possible to deduce oscillator strengths for 129 transitions of Os I and 137 transitions of Os II of astrophysical interest appearing in the wavelength range 180.0-870.0 nm. These results have allowed us to revise the abundance of osmium in the solar photosphere (log \varepsilonOs = 1.25 ± 0.11). The newly derived oscillator strengths have been applied as well to derive the osmium abundance in the carbon-rich metal-poor star HD 187861.

Affiliated with

Also associated with

No associations

Rating

Transition probabilities and lifetimes in neutral and singly ionized osmium and the Solar osmium abundance 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 Transition probabilities and lifetimes in neutral and singly ionized osmium and the Solar osmium abundance, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Transition probabilities and lifetimes in neutral and singly ionized osmium and the Solar osmium abundance will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1579207