| Numéro |
J. Phys. Colloques
Volume 49, Numéro C1, Mars 1988
IAU Colloquium N° 102 on UV and X-ray Spectroscopy of Astrophysical and Laboratory Plasmas
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|---|---|---|
| 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
Physics Department, AMU, Aligarh-202001. India
J. Phys. Colloques 49 (1988) C1-239-C1-239
DOI: 10.1051/jphyscol:1988149
VUV SPECTRA Y TO Mo
M.S.Z. CHAGHTAIPhysics 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.