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J/A+AS/115/351 Stark broadening. XIII. C V and P V (Dimitrijevic+, 1996)
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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)
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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:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table1 124 1530 Stark broadening parameters due to e-, p-
and He III-impacts for C V and P V
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See also:
VI/82 : Stark broadening of H lines
J/A+AS/105/243 : Stark broadening of BeI lines
J/A+AS/105/245 : Stark broadening of Al XI and Si XII
J/A+AS/107/349 : Stark broadening of Ne VIII and Na IX
J/A+AS/109/551 : Stark broadening of OIV and OV
J/A+AS/116/359 : Stark broadening of Xe II lines
J/A+AS/117/127 : Stark broadening of solar MgI lines
J/A+AS/119/369 : Stark broadening of Be III and B III
J/A+AS/119/529 : Stark broadening of Sr I spectral lines
J/A+AS/120/373 : Stark width in Sc II, Y II and Zr II spectra
J/A+AS/122/163 : Stark broadening of Ba I and Ba II lines
J/A+AS/122/533 : Stark broadening of P IV spectral lines
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)
Byte-by-byte Description of file: table1
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Bytes Format Units Label Explanations
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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)
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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
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(End) Simona Mei [CDS] 13-Oct-1995
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