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Detailed Description of J/A+AS/140/193
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Individual files can be fetched (via http) from
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This standardized document follows the rules of the Standard Description for Astronomical Catalogues. For those having to work on this catalogue using FORTRAN programs, this ReadMe file can be transformed into a f77-compliant program which reads the files making up this catalogue, in two versions: either a f77 program loading whole files into arrays, or a f77-program reading each data file line by line.
J/A+AS/140/193 Stark broadening of Zn I (Dimitrijevic+, 1999)
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Stark broadening of neutral zinc spectral lines
Dimitrijevic M.S., Sahal-Brechot S.
<Astron. Astrophys. Suppl. Ser. 140, 193 (1999)>
=1999A&AS..140..193D
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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
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(End) Patricia Bauer [CDS] 09-Sep-1999
