... sterne . f77 . Model atmospheres in LTE . spectrum . f77 . LTE radiative transfer . ... Fit hires spectrum for Teff, log g, n_i, v sin i, for single and binary stars. n_i ...
... spectrum specm=fltarr(nwave) FOR iw=0,nwave-1 DO BEGIN specm(iw) = median(spec(iw,0:nspec-1)) ENDFOR cont = fltarr(nwave,nspec) ;; define continuum regions ncont = n_elements(creg) creg_loc = where(wave ge creg(0) and wave le creg(1)) FOR ic = 0,ncont-1,2 ...
... spectrum specm = fltarr(nwave) FOR iw = 0,nwave-1 DO specm(iw) = mean(specf(iw,*)) ; Bale out here if this is a models and cleaning was not requried if (keyword_set(model)) then return if (n_elements(nwomit) EQ 0) THEN nwomit = 0 FOR iw = nwomit,nwave-1 ...
... Figure 4. The X-ray spectrum of KL Dra observed during the faint optical state. ... There is some evidence for a spectral evolution of the X-ray spectrum during the course of the outburst. ...
... Within a few percents, no variation in Iris' visible spectrum over a rotational period has been found. ... Taking into account the close similarity between Iris' spectrum and that of (6) Hebe, a typical S(IV)-type object according ...
... the family, we report on our own observations of the optical reflectance spectrum of Hoffmeister, carried out with the 1.54~m ... The spectrum has been found to be flat and featureless over the whole wavelength range between about 5200 and 9000 {\AA ...
... Two attempts were made to detect the spectrum of the secondary at, respectively, the ... low-luminosity companion in either the integrated spectrum or in a cross-correlation ...
... Observed spectrum and model spectrum of temperature 38kK, log g 4.5 cms-2 and helium 99% . ... This model spectrum fitted my observed spectrum best. ...
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Ссылки http://star.arm.ac.uk/~csj/nuffield/posters/2012_McCARNEY.pdf -- 464.5 Кб -- 11.09.2012 Похожие документы