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J/A+AS/115/351      Stark broadening. XIII. C V and P V   (Dimitrijevic+, 1996)
Stark broadening spectral lines of multicharged ions of astrophysical
interest. XIII. C V and P V
     Dimitrijevic M.S., Sahal-Brechot S.
    <Astron. Astrophys. Suppl. Ser. 115, 351 (1996)>
    =1996A&AS..115..351D      (SIMBAD/NED BibCode)
ADC_Keywords: Atomic physics

Keywords: line: profiles - atomic and molecular data


Description:
    Using a semiclassical approach, we have calculated electron-, proton-,
    and He III-impact line widths and shifts for 25 C V and 51 P V
    multiplets.

File Summary:

       FileName      Lrecl  Records   Explanations

ReadMe            80        .   This file
table1           124     1530   Stark broadening parameters due to e-, p-
                                 and He III-impacts for C V and P V


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/116/359 : Xe II lines (Popovic+, 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/400/791  : Be III (Dimitrijevic+ 2003)
      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-  7  E7.2  cm-3       N         Perturber density
  12- 15  A4    ---        El        Element
  18- 22  A5    ---        Tr        Transition
  24- 30  F7.1  0.1nm      Lambda    Wavelength
  33- 40  E8.2  0.1nm/cm3  C         Parameter C (1)
  43- 49  I7    K          T         Temperature
      52  A1    ---        n_We      [*] See note (4)
  53- 61  E9.3  0.1nm      We        ? FWHM for electron impacts (2)
      64  A1    ---        n_de      [*] See note (4)
  65- 74  E10.3 0.1nm      de        ? Shift for electron impacts (3)
      77  A1    ---        n_Wp      [*] See note (4)
  78- 86  E9.3  0.1nm      Wp        ? FWHM for proton impacts (2) (5)
      89  A1    ---        n_dp      [*] See note (4)
  90- 99  E10.3 0.1nm      dp        ? Shift for proton impacts (3) (5)
     102  A1    ---        n_WHe++   [*] See note (4)
 103-111  E9.3  0.1nm      WHe++     ? FWHM for He III-impacts (2)
     114  A1    ---        n_dHe++   [*] See note (4)
 115-124  E10.3 0.1nm      dHe++     ? Shift for He III-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

(End)                                        Simona Mei [CDS]   13-Oct-1995