Access to Astronomical Catalogues

← Click to display the menu
J/A+AS/140/193      Stark broadening of Zn I               (Dimitrijevic+, 1999)

Stark broadening of neutral zinc spectral lines Dimitrijevic M.S., Sahal-Brechot S. <Astron. Astrophys. Suppl. Ser. 140, 193 (1999)> =1999A&AS..140..193D
ADC_Keywords: Atomic physics Keywords: atomic data - line profiles Abstract: Using the semiclassical perturbation approach, we have calculated electron-, proton- and He II-impact line widths and shifts for 32 Zn I multiplets as a function of temperature and perturber density. Obtained results have been compared with the existing theoretical and experimental data File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 123 594 Stark broadening parameters due to e-, p- and He II-impacts for Zn I for perturber densities 1.E+13cm-3 - 1.E+19cm-3.
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/133/227 : K VIII and K IX (Dimitrijevic+ 1998) J/A+AS/140/191 : Ca 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
Bytes Format Units Label Explanations
1- 7 E7.2 cm-3 N Perturber density 10- 13 A4 --- El [Zn I] Element 16- 21 A6 --- Tr Transition (4) 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 [*] See note (5) 53- 61 E9.3 0.1nm We FWHM for electron impacts (2) 63 A1 --- n_de [*] See note (5) 64- 73 E10.3 0.1nm de Shift for electron impacts (3) 76 A1 --- n_Wp [*] See note (5) 77- 85 E9.3 0.1nm Wp FWHM for proton impacts (2) (6) 88 A1 --- n_dp [*] See note (5) 89- 98 E10.3 0.1nm dp Shift for proton impacts (3) (6) 101 A1 --- n_WHe+ [*] See note (5) 102-110 E9.3 0.1nm WHe+ FWHM for He II-impacts (2) 113 A1 --- n_dHe+ [*] See note (5) 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): In the first part of the Table are singlets and in the second triplets Note (5): 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 (6): 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] 09-Sep-1999
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

catalogue service

© UDS/CNRS

Contact