J/A+AS/120/373      Sc II, Y II & Zr II Stark width (Popovic+ 1996)

Stark width for astrophysically important ns-np transitions in Sc II, Y II and Zr II spectra. Popovic L.C., Dimitrijevic M.S. <Astron. Astrophys. Suppl. Ser. 120, 373 (1996)> =1996A&AS..120..373P 1996A&AS..120..373P (SIMBAD/NED BibCode)
ADC_Keywords: Atomic physics Keywords: atomic data - lines: profiles Abstract: Here we present Stark widths for some astrophysically important ns-np transitions of Sc II, Y II and Zr II. Stark widths were calculated within the modified semiempirical approach. The obtained results were compared with simple estimates based on regularities and systematic trends. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1-3 50 108 *Stark full width (FWHM) for Sc II, Y II and Zr II spectral lines tables.tex 76 213 TeX version of table1-3 -------------------------------------------------------------------------------- Note to table1-3: The electron density is 10+23 m-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/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: table1-3 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 A5 --- Ion Ion 7- 26 A20 --- Trans Transition 29- 33 F5.1 nm Lambda Wavelength 34 A1 --- n_Lambda [a] a stands for averaged wavelength of the multiplet 36- 40 I5 K T Temperature 43- 50 E8.3 nm W Stark width -------------------------------------------------------------------------------- Acknowledgements: Dr. Luka C. Popovic
(End) Patricia Bauer [CDS] 24-May-1996
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