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J/A+AS/107/349 Stark broadening X. (Dimitrijevic+, 1994)
Stark broadening of spectral lines of multicharged ions of astrophysical interest X: Ne VIII and Na IX Dimitrijevic M.S., Sahal-Brechot S. <Astron. Astrophys. Suppl. Ser. 107, 349 (1994)> =1994A&AS..107..349D (SIMBAD/NED Reference)
ADC_Keywords: Atomic physics Keywords: line: profiles - atomic and molecular data File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1 123 350 Stark broadening parameters due to e-, p- and He III-impacts for Ne VIII and Na 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/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/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
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 52 A1 --- n_We [*] Note on We (4) 53- 61 E9.3 0.1nm We FWHM for electron impacts (2) 63 A1 --- n_de [*] Note on de (4) 64- 73 E10.3 0.1nm de shift for electron impacts (3) 76 A1 --- n_Wp [*] Note on Wp (4) 77- 85 E9.3 0.1nm Wp []? FWHM for proton impacts (2) (5) 88 A1 --- n_dp [*] Note on dp (4) 89- 98 E10.3 0.1nm dp []? shift for proton impacts (3) (5) 101 A1 --- n_WHe++ [*] Note on WHe++ (4) 102-110 E9.3 0.1nm WHe++ []? FWHM for He III-impacts (2) 113 A1 --- n_dHe++ [*] Note on dHe++ (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 < 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
Courtesy: Sylvie Sahal-Brechot & Milan S. Dimitrijevic
(End) Patricia Bauer [CDS] 26-May-1994
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