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J/A+AS/116/359      Xe II lines Stark broadening (Popovic+, 1996)
Stark broadening of Xe II lines.
     Popovic L.C., Dimitrijevic M.S.
    <Astron. Astrophys. Suppl. Ser. 116, 359 (1996)>
    =1996A&AS..116..359P      (SIMBAD/NED BibCode)
ADC_Keywords: Atomic physics

Keywords: atomic data - plasmas - stars: chemically peculiar


Description:
    We present here Stark widths and shifts for 20 Xe II multiplets which
    are of interest for laboratory plasma research as well as for the
    analysis of Hg-Mn stars spectra. For calculations the modified
    semiempirical approach was used. The obtained results are compared
    with the available experimental data.

File Summary:

       FileName      Lrecl  Records   Explanations

ReadMe            80        .   This file
table1            61      120  *Stark full widths and shifts of Xe II lines
table1.tex        79      466   LaTeX version of table1
table2            73      124   Comparison of measured and theoretical values
                                  for Stark widths and shifts
table2.tex        79      614   LaTeX version of table2

Note on table1: The electron density is 1E23 m(-3). The averaged wavelength of
  the multiplet is denoted by overlined lambda


See also:
               VI/98 : Stark broadening of H lines (Stehle+, 1999)
  Stark broadening of other elements (Dimitrijevic, Sahal-Brechot, Popovic)

      J/A+AS/105/243 : BeI lines (Dimitrijevic+ 1994)
      J/A+AS/105/245 : Al XI and Si XII (Dimitrijevic+ 1994)
      J/A+AS/107/349 : Ne VIII and Na IX (Dimitrijevic+ 1994)
      J/A+AS/109/551 : OIV and OV (Dimitrijevic+ 1995)
      J/A+AS/115/351 : C V and P V (Dimitrijevic+, 1996)
      J/A+AS/117/127 : solar Mg I lines (Dimitrijevic+, 1996)
      J/A+AS/119/369 : Be III and B III (Dimitrijevic+, 1996)
      J/A+AS/119/529 : Sr I spectral lines (Dimitrijevic+, 1996)
      J/A+AS/120/373 : Sc II, Y II and Zr II Stark width (Popovic+ 1996)
      J/A+AS/122/163 : Ba I and Ba II lines (Dimitrijevic+, 1996)
      J/A+AS/122/533 : P IV spectral lines (Dimitrijevic+, 1997)
      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)
      J/A+A/417/375  : Cd III (Milovanovic+, 2004)
      J/A+A/423/397  : Si V (Ben Nessib+, 2004)
      J/A+A/425/1147 : Ga I (Dimitrijevic+, 2004)


Byte-by-byte Description of file: table1

   Bytes Format Units   Label     Explanations

   1- 29  A29   ---     Trans     Transition
  31- 35  F5.1  nm      Lam       Wavelength
  38- 42  I5    K       T         Temperature
  44- 51  E8.3  nm      W         Stark width
  53- 61  E9.3  nm      d         Stark shift


Byte-by-byte Description of file: table2

   Bytes Format Units   Label     Explanations

   1- 29  A29   ---     Trans     Transition
  31- 36  F6.2  nm      Lam       Wavelength
  38- 41  F4.1  1000K   T         Temperature
  43- 48  F6.4  nm      Wm        []? Measured Stark width
      49  A1    ---     l_dm      Limit flag on dm
  50- 57  F8.5  nm      dm        []? Measured Stark shift
  59- 61  F3.1  ---     Wm/Wth    []? Measured versus theoretical Stark width
  63- 65  F3.1  ---     dm/dth    []? Measured versus theoretical Stark shift
      67  A1    ---     n_dm/dth  [*] Note on dm/dth (1)
  71- 72  I2    ---     Ref       References

Note (1): When *, the measured and the calculated values of Stark shift
          have different sign


References:
  (1) Nick K. P., Helbig, 1986, Phys. Scr. 33, 55
  (2) Di Rocco H. O., 1990b, Il Nuovo Cimento 12D, 1485
  (3) Gigosos M. A., Mar S., Perez C. and I. de la Rosa, 1994,
       Phys. Rev. E49, 1575
  (4) Lesage A., Miller M. H., Richou J., Bach T., 1981, in Spectral Line
       Shapes, Ed. B. Wende,  W. de Gruyter, Berlin, New York, p. 257
  (5) Lesage A., Abadie D., Miller M. H., 1989, Phys. Rev. A 40, 1367
  (6) Miller M. H., Lesage A., Abadie D., 1981, Phys. Rev. A 25, 2064
  (7) Bertuccelli D., Bertuccelli G., Di Rocco H. O., 1991, Phys. Scr. 43, 469
  (8) Richou J., Manola S., Lebrun J. L., Lesage A, 1984, Phys. Rev. A29, 3181
  (9) Vitel Y., Skowronek M., 1987, J. Phys. B 20, 6493
 (10) Konjevi'c N., Uzelac N. I., 1990, JQSRT 44, 61
 (11) Manola et al. 1988, Phys. Rev. A38, 5742
(End)                                           Patricia Bauer [CDS] 16-Jan-1996