We present calculations of the oscillator strengths of Fe ii ll2507, 2509, which are the strongest observed lines in the emission spectrum of the B and D Weigelt blobs of h Carinae. Unlike previous determinations of these oscillator strengths, our results are compatible with the modeling undertaken by Verner et al.

No abstract

We present extensive configuration interaction calculations of oscillator strengths and transition rates of certain near-infrared emission lines of Fe ii observed in the BD Weigelt blobs of Carinae. Comparison is made between our work and results available in existing databases. We offer arguments in favor of our results being the most accurate, where differences occur.

No abstract