Access to Astronomical Catalogues

← Click to display the menu
J/A+AS/105/245    Stark broadening Al XI and Si XII   (Dimitrijevic+ 1994)

Stark broadening of spectral lines of multicharged ions of astrophysical interest. XI: Al XI and Si XII Dimitrijevic M.S., Sahal-Brechot S. <Astron. Astrophys. Suppl. Ser. 105, 245 (1994)> =1994A&AS..105..245D
ADC_Keywords: Atomic physics Keywords: line: profile - atomic data 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/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+AS/140/193 : Zn I (Dimitrijevic+ 1999) J/A+A/389/716 : Oscillator strengths for Li-like ions (Nahar, 2002) 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) File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1 124 308 Stark broadening parameters due to e-, p- and He III-impacts for Al XI and Si XII
Byte-by-byte Description of file: table1
Bytes Format Units Label Explanations
1- 7 E7.2 cm-3 N Perturber density 10- 15 A6 --- 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- 50 F8.0 K T Temperature 53- 61 E9.3 0.1nm We FWHM for electron impacts (2) 64- 73 E10.3 0.1nm de shift for electron impacts (3) 76 A1 --- n_Wp [*] (4) 77- 85 E9.3 0.1nm Wp []? FWHM for proton impacts (2) (5) 88 A1 --- n_dp [*] (4) 89- 98 E10.3 0.1nm dp []? shift for proton impacts (3) (5) 101 A1 --- n_WHe++ [*] (4) 102-110 E9.3 0.1nm WHe++ []? FWHM for He III-impacts (2) (5) 113 A1 --- n_dHe++ [*] (4) 114-123 E10.2 0.1nm dHe++ []? shift for He III-impacts (3) (5)
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 the 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 < N V < 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 N V > 0.5 are not given, because in this case the impact approximation is no longer valid

(End) Sylvie Sahal-Brechot [Meudon], Patricia Bauer [CDS] 17-Feb-1994
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