(1) Mount Wilson and Palomar Observatories, Carnegie Institution of Washington, Pasadena, Calif., U.S.A.;(2) California Institute of Technology, Pasadena, Calif., U.S.A.;(3) Dept. of Astrophysics, University of Oxford, Oxford, England
Abstract:
New observations of the Caii] 7323 Fraunhofer line are reported. The blending H2O line was weak at the time of observation. Accurate estimates of the centre-limb variation of the equivalent width of the Caii] transition are obtained and shown to be consistent with the calcium abundance log N(Ca) = 6.33.