/ftp/cats/J_A+AS/113/579



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J/A+AS/113/579                             Stark broadening  (Shoening+, 1995)
The following files can be converted to FITS (extension .fit .fit.Z .fgz)
	table1 table2
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Query from: http://vizier.u-strasbg.fr/cgi-bin/VizieR?-source=J/A+AS/113/579
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drwxr-xr-x 18 cats archive 4096 Jan 29 2012 [Up] drwxr-xr-x 2 cats archive 4096 May 12 09:56 [TAR file] -rw-r--r-- 1 cats archive 470 Dec 9 1997 .message -rw-r--r-- 1 cats archive 4460 Oct 28 1997 ReadMe -rw-r--r-- 1 cats archive 213 Sep 19 2007 +footg5.gif -rw-r--r-- 1 cats archive 2047 Mar 5 2008 +footg8.gif -r--r--r-- 1 cats archive 59013 Jun 8 1995 table1 -r--r--r-- 1 cats archive 27255 Jun 8 1995 table2
Beginning of ReadMe : J/A+AS/113/579 Stark broadening (Shoening+, 1995) ================================================================================ Stark broadening of the NV 6f,g,h-7f,g,h,i line complex SCHOENING T. <Astron. Astrophys. Suppl. Ser. 113, 579 (1995)> =1995A&AS..113..579S (SIMBAD/NED BibCode) ================================================================================ ADC_Keywords: Atomic physics; Line Profiles Keywords: atomic data - line: profiles - plasmas - stars: abundances Description: Tables of Stark broadening profiles for the N V 6f, g, h-7f, g, h, i line complex at 4945A have been generated. Modern close-coupling techniques are used for the electron broadening while the important influence of perturbing ions is included within the framework of the model microfield method. Comparison has been made with the results of line formation calculations using approximate formulae for the Stark profiles.

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