/ftp/cats/6/39



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VI/39  MODEL ATMOSPHERE FOR G, F, A, B, AND O STARS
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Query from: http://vizier.cds.unistra.fr/cgi-bin/VizieR?-source=VI/39
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drwxr-xr-x 141 cats archive 4096 Sep 6 2023 [Up] drwxr-xr-x 2 cats archive 319 Aug 3 2023 [TAR file] -rw-r--r-- 1 cats archive 347 Dec 19 2022 .message -r--r--r-- 1 cats archive 3895 Jan 24 1999 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 3974222 May 16 1991 main.gz [Uncompressed] -r--r--r-- 1 cats archive 5104 Oct 14 1993 models.gz [Uncompressed] -rw-r--r-- 1 cats archive 1840 Feb 17 1995 note.dvi -r--r--r-- 1 cats archive 943 Oct 14 1993 note.tex -r--r--r-- 1 cats archive 1151 Oct 14 1993 readfile.f
Beginning of ReadMe : VI/39 Model Atmospheres (Kurucz, 1979) ================================================================================ Model Atmosphere for G, F, A, B, and O stars Kurucz R.L. <Astrophys. J. Suppl. Ser. 40, 1 (1979)> =1979ApJS...40....1K (SIMBAD/NED RefCode) ================================================================================ ADC_Keywords: Models, atmosphere Description of the tape by Robert Kurucz: This tape lists fluxes and temperature-mass relations for 1200 models. The first 284 models are from Kurucz, R.L., Ap.J. Supp., 40,1,1979 and are described there. Next are purely radiactive models for A and B stars with Teff 8000K to 20000K for [M/H] =-1.,-.5,+.5,+1. Finally are new improved convective models for 5500K to 8500K with [M/H]=+1.,+.5,0.,-.5,-1.,-1.5, -2.,-2.5,-3.,-9.99. Because the new models have not yet been published and because I am computing visible and infrared colors in various photometric systems, these new fluxes should not be used to publish colors without my agreement. For any other use these fluxes are in the public domain. The models are presented as ATLAS format input decks. The tape is recorded on 9 tracks at 1600 bpi in ASCII card images with 4000 character blocks. A sample program that reads the tape follows. I suggest that the user read the tape once and write a binary tape that can be read much more quickly. Program to read the tape: PROGRAM FLUXREAD DIMENSION WAVE(342),HNU(342),CONT(342) DIMENSION C(20) DO 2 I=1,6 READ(1,1)C 1 FORMAT(20A4) 2 PRINT 1,C READ(1,3)WAVE 3 FORMAT(8F10.1) PRINT 3,WAVE DO 6 MODEL=1,1200 READ(1,4)TEFF,GRAV,ABUND 4 FORMAT(F7.0,F6.2,F6.2) PRINT 11,MODEL,TEFF,GRAV,ABUND 11 FORMAT(I5,F7.0,F6.2,F6.2) READ(1,5)HNU,CONT 5 FORMAT(7E11.4) 6 CONTINUE C MODELS DO 13 MODEL=1,1200 READ(1,1)C PRINT 9,MODEL,C 9 FORMAT(I5,20A4) NUM=45 IF(MODEL.GT.609) NUM=69 DO 12 I=2,NUM 12 READ(1,1)C 13 CONTINUE STOP END Parameters from Table 6 and Table 4 See the enclosed note.tex (standard latex) for units in Table 6. The enclosed program readfile.f (standard f77) based on the above program reads the input file (assumed logical unit 5) and prints the values from Table 6 and headers of Table 4 A file (grid) which contains the basic parameters of the the 1200 models has been directly created from the main file.