Issue
J. Phys. Colloques
Volume 49, Number C1, Mars 1988
IAU Colloquium N° 102 on UV and X-ray Spectroscopy of Astrophysical and Laboratory Plasmas
Page(s) C1-239 - C1-239
DOI https://doi.org/10.1051/jphyscol:1988149
IAU Colloquium N° 102 on UV and X-ray Spectroscopy of Astrophysical and Laboratory Plasmas

J. Phys. Colloques 49 (1988) C1-239-C1-239

DOI: 10.1051/jphyscol:1988149

VUV SPECTRA Y TO Mo

M.S.Z. CHAGHTAI

Physics Department, AMU, Aligarh-202001. India


Abstract
Using R.D. Cowan's computations (1979) and parametric calculations of Weinders et al (1982), old analyses are thoroughly revised and extended at Aligarh, of Zr III by Khan et al (1981), of Wb IV by Shujauddin et Chaghtai (1985), of Mo V by Tauheed et al (1985). Cabeza et al (1986) confirmed the last one largely.