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J/A+AS/133/227      Stark broadening of K VIII and K IX (Dimitrijevic+ 1998)

Stark broadening of spectral lines of multicharged ions of astrophysical interest. XXII: K VIII and K IX spectral lines Dimitrijevic M.S., Sahal-Brechot S. <Astron. Astrophys. Suppl. Ser. 133, 227 (1998)> =1998A&AS..133..227D (SIMBAD/NED BibCode)
ADC_Keywords: Atomic physics Keywords: atomic data - line profiles Abstract: By using the semiclassical-perturbation formalism, we have calculated electron-, proton-, and He III-impact line widths and shifts for 4 K VIII and 30 K IX multiplets, of interest for analysis, investigation and modeling of different plasmas in solar and stellar subphotospheric layers research and plasma physics. The obtained results are presented as a function of temperature and perturber density. Results are compared with other theoretical estimates, based on regularities and systematic trends. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 123 108 Stark broadening parameters due to e-, p- and He III-impacts for K VIII table2.dat 123 720 Stark broadening parameters due to e-, p- and He III-impacts for K IX
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/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/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.dat table2.dat
Bytes Format Units Label Explanations
1- 7 E7.2 cm-3 N Perturber density 9- 13 A5 --- El Element 15- 20 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 [*] Validity flag (4) 53- 61 E9.3 0.1nm We FWHM for electron impacts (2) 63 A1 --- n_de [*] Validity flag (4) 64- 73 E10.3 0.1nm de shift for electron impacts (3) 76 A1 --- n_Wp [*] Validity flag (4) 77- 85 E9.3 0.1nm Wp FWHM for proton impacts (2) (5) 88 A1 --- n_dp [*] Validity flag (4) 89- 98 E10.3 0.1nm dp shift for proton impacts (3) (5) 101 A1 --- n_WHe++ [*] Validity flag (4) 102-110 E9.3 0.1nm WHe++ FWHM for He III-impacts (2) 113 A1 --- n_dHe++ [*] Validity flag (4) 114-123 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
Acknowledgements: Dr Milan Dimitrijevic
(End) Patricia Bauer [CDS] 08-Jun-1998
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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