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J/A+AS/119/369     Stark broadening. XIV: Be III and B III (Dimitrijevic+, 1996)
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Stark broadening of spectral lines of multicharged ions of astrophysical
interest. XIV: Be III and B III.
     Dimitrijevic M.S., Sahal-Brechot S.
    <Astron. Astrophys. Suppl. Ser. 119, 369 (1996)>
    =1996A&AS..119..369D      (SIMBAD/NED BibCode)
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ADC_Keywords: Atomic physics
Keywords: atomic and molecular data - line: profiles

Description:
    Using a semiclassical approach, we have calculated electron-, proton-,
    and ionized helium-impact line widths and shifts for 12 Be III and 27
    B III multiplets. The obtained results have been compared with
    available experimental and theoretical data.

File Summary:
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  FileName      Lrecl  Records   Explanations
--------------------------------------------------------------------------------
ReadMe             80        .   This file
table1            123      594   Stark broadening parameters due to e-, p- and
                                  He II-impacts for Be III and B III
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See also:
                   VI/82 : Stark broadening of H lines
          J/A+AS/105/243 : Stark broadening of BeI lines
          J/A+AS/105/245 : Stark broadening Al XI and Si XII
          J/A+AS/107/349 : Stark broadening of Ne VIII and Na IX
          J/A+AS/109/551 : Stark broadening of OIV and OV
          J/A+AS/115/351 : Stark broadening of C V and P V
          J/A+AS/116/359 : Stark broadening of Xe II lines
          J/A+AS/119/529 : Stark broadening of Sr I spectral lines
          J/A+AS/120/373 : Stark width in Sc II, Y II and Zr II spectra
          J/A+AS/122/163 : Stark broadening of Ba I and Ba II lines
          J/A+AS/122/533 : Stark broadening of P IV spectral lines
          J/A+AS/127/295 : Kr II lines (Popovic+ 1998)
          J/A+AS/127/543 : S V lines (Dimitrijevic+ 1998)
          J/A+AS/128/203 : Mn, Ga & Ge multiplets (Popovic+ 1998)
          J/A+AS/128/359 : Ca IX and Ca X lines (Dimitrijevic+ 1998)
          J/A+AS/129/155 : Si XI and Si XIII lines (Dimitrijevic+ 1998)
          J/A+AS/130/539 : Na X (Dimitrijevic+ 1998)
          J/A+AS/131/141 : O VII and Mg XI (Dimitrijevic+ 1998)
          J/A+AS/131/143 : Sc X, Sc XI, Ti XI and Ti XII (Dimitrijevic+ 1998)
          J/A+AS/133/227 : K VIII and K IX (Dimitrijevic+ 1998)
          J/A+AS/140/191 : Ca I (Dimitrijevic+ 1999)
          J/A+AS/140/193 : Zn I (Dimitrijevic+ 1999)

Byte-by-byte Description of file: table1
--------------------------------------------------------------------------------
   Bytes Format     Units   Label     Explanations
--------------------------------------------------------------------------------
   1-  7  E7.2      cm-3    N         Perturber density
  10- 15  A6        ---     El        Element name
  17- 22  A6        ---     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        [*] (4)
  53- 61  E9.3      0.1nm   We        FWHM for electron impacts (2)
      63  A1        ---   n_de        [*] (4)
  64- 73  E10.3     0.1nm   de        shift for electron impacts (3)
      76  A1        ---   n_Wp        [*] (4)
  77- 85  E9.3      0.1nm   Wp        FWHM for proton impacts (2) (5)
      88  A1        ---   n_dp        [*] (4)
  89- 98  E10.3     0.1nm   dp        shift for proton impacts (3) (5)
     101  A1        ---   n_WHe+      [*] (4)
 102-110  E9.3      0.1nm   WHe+      FWHM for He II-impacts (2)
     113  A1        ---   n_dHe+      [*] (4)
 114-123  E10.3     0.1nm   dHe+      shift for He II-impacts (3)
--------------------------------------------------------------------------------
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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Courtesy: Milan S. Dimitrijevic <mdimitrijevic@aob.aob.bg.ac.yu>
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(End)                                         Patricia Bauer [CDS]   02-Apr-1996

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