October 12, 2021
Author(s)
C R. Proffitt, T Brage, D S. Leckrone, G Wahlgren, J C. Brandt, Craig J. Sansonetti, Joseph Reader, S Johansson
… are present, with UV Hg I lines being too weak, and Hg III lines too strong for the abundance derived from lines of … effect, but the same non-LTE calculations show that the Hg III ionizaiton anomaly in chi Lupi cannot be explained in … of the order of 10- 14 M(solar) yr-1 supports a cloud of g III at very small optical depths. …