J/A+A/441/391       Stark broadening of Cd I spectral lines      (Simic+, 2005)
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Stark broadening of Cd I spectral lines.
    Simic Z., Dimitrijevic M.S., Milovanovic N., Sahal-Brechot S.
   <Astron. Astrophys. 441, 391 (2005)>
   =2005A&A...441..391S
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ADC_Keywords: Atomic physics
Keywords: atomic data - line profiles

Abstract:
    Stark broadening parameters, widths, and shifts for 33 CdI singlets
    and 37 triplets were calculated using the semiclassical perturbation
    method. The results were compared with available experimental and
    theoretical data. Also, regularity in the spectral series
    5s^2^ ^1^S-np ^1^P^o^ was investigated. The influence of Stark
    broadening was analyzed in A-type stellar atmospheres.

File Summary:
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 FileName  Lrecl  Records   Explanations
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ReadMe        80        .   This file
table1.dat   123      582   Stark broadening parameters due to e-, p- and
                             He II-impacts for Cd I singlets for perturber
                             densities 10^+13^cm^-3^-10^+19^cm^-3^.
table2.dat   123      558   Stark broadening parameters due to e-, p- and
                             He II-impacts for Cd I triplets for perturber
                             densities 10^+14^cm^-3^-10^+18^cm^-3^.
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See also:
   J/A+A/417/375 : Cd III Stark broadening parameters (Milovanovic+, 2004)

Byte-by-byte Description of file: table1.dat table2.dat
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   Bytes Format Units    Label     Explanations
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   1-  7  E7.2  cm-3     N         Perturber density
  10- 13  A4    ---      El        Element
  14- 22  A9    ---      Tr        Transition
  23- 30  F8.1  0.1nm    lambda    Wavelength
  33- 40  E8.2 0.1nm/cm3 C         Parameter C (1)
  43- 50  F8.0  K        T         Temperature
      52  A1    ---    n_We        [*] Note on We (4)
  53- 61  E9.3  0.1nm    We        ? FWHM for electron impacts (2)
      63  A1    ---    n_de        [*] Note on de (4)
  64- 73  E10.3 0.1nm    de        ? Shift for electron impacts (3)
      76  A1    ---    n_Wp        [*] Note on Wp (4)
  77- 85  E9.3  0.1nm    Wp        ? FWHM for proton impacts (2) (5)
      88  A1    ---    n_dp        [*] Note on dp (4)
  89- 98  E10.3 0.1nm    dp        ? Shift for proton impacts (3) (5)
     101  A1    ---    n_WHe+      [*] Note on WHe+ (4)
 102-110  E9.3  0.1nm    WHe+      ? FWHM for He II-impacts (2)
     113  A1    ---    n_dHe+      [*] Note on dHe+ (4)
 114-123  E10.3 0.1nm    dHe+      ? Shift for He II-impacts (3)
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Note (1): C/FWHM gives an estimate of the maximum perturber density for which
          the line may be treated as isolated and tabulated data may be used.
Note (2): FWHM denotes Full Width at Half Maximum
Note (3): A positive (resp. negative) shift is towards the red (resp. blue)
Note (4): An asterisk in this column indicates that 0.1<NV<0.5,
          (V = collision volume); beware of the fact that the limit of validity
          of the impact approximation  is attained for the value that follows
Note (5): Values for NV>0.5 are not given, because in this case the impact
          approximation is no longer valid
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Acknowledgements: Milan Dimitrijevic, mdimitrijevic(at)aob.bg.ac.yu
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(End)                                      Patricia Vannier [CDS]    19-Sep-2005
