October 16, 2008
Author(s)
U I. Safronova, I Murakami, T Kato, D Kato, Y Ralchenko
Energy levels, radiative transition probabilities, and autoionization rates for C-like oxygen (O$^2+}$) including $1s^22s^22pnl$, $1s^22s2p^2nl$, and $1s^22p^3nl$ ($n$=2-8, $l \le n-1$) states are calculated by theHartree-Fock-Relativistic method (Cowan