“…Notable differences from Warner's [82] results for Ti I1 and V I1 were found, and this fact may necessitate a substantial increase of the presently adopted photospheric abundances of these elements. Also for Cr I and Ni I radiative lifetimes have been measured in this way, by Cocke et al [86], Brand et al [87], and Lennard et al [88]. Preliminary values for lifetimes in Cr I, Cr 11, Mn I, Mn 11, Mn 111, CO I and CO I11 have been presented by Pinnington et al [89], whereas Martinson et al [go] reported lifetimes for a number of Mn I and Mn I1 terms.…”