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1、___________________________________________________________SchemeforGRASILparametersandusage___________________________________________________________(1)ListoffilestorunGRASILSourcefiles:gsuti.f90,grasil.f90,gslight.f90,gsmain.f90,gsmol3.f90,gshii3.f90,gsflut.f90,gsd
2、iff.f90,gspah.f90,lvgdatos.f90,lvgsubruti.f90,dfport.f90,taututto.f90,tauflut.f90,tausub.f90,taujd.f90,taumod.f90,tausto.f90,taupah.f90,mstarsub.f90,num.f90,q_draine.f90,graann.f90,network.f90,precismod.f90,utilmod.f90Executables(forWindowsandLinux):grasil(orgrasil_wi
3、n.exe,grasil_linux)SampleshelltocompilewithIntelcompilerforLinux:compall.tcshInputfilestorunGRASIL:·GRA_81,SIL_81,sigmapah_07.dat,TAU96.OF:variousfilesneededbyGRASILfordustproperties.Mustbeinthesamedirectoryastheexecutable·FilesforSSPs:Thesetoomustbeinthesamedirectory
4、astheexecutable.SSPfileswithextensions*.sal,*.ken,*.msc,*.kro,*.scm,*.chaidentifytheIMFwithwhichtheSSPshavebeencomputed(respectivelySalpeter,Kennicutt,Miller&Scalo,Kroupa,“modifiedScalo”,Chabrier,moredetailsbelow).ForeachIMF,there’soneSSPfileforeachmetallicity,contain
5、ingtheSEDforalargerangeofages.TheSSPsdescribedbelowarebasedontheKuruczstellarlibrary,coveraquitelargerangeofIMFs,andarecomputedforstellarmassesfrom0.15to120Mo.TheyalsoincludethedustemissionfromAGBdustyenvelopes(seeBressan,Granato,Silva1998)andradioemission(boththermal
6、andsynchrotron,seeBressan,Silva,Granato2002).IfnecessarySSPswithhigherresolutionandmoreIMFsareavailable.Specifically:SalpeterIMF():gsrdk0bZ0004.sal,gsrdk0bZ004.sal,gsrdk0bZ008.sal,gsrdk0bZ02.sal,gsrdk0bZ05.salKennicuttIMF(forM£1,forM>1):gkn15rdZ0004.ken,gkn15rdZ004.ke
7、n,gkn15rdZ008.ken,gkn15rdZ02.ken,gkn15rdZ05.kenModifiedKennicutt-typeIMF(forM£1,forM>1):gkn1rdZ0004.ken,gkn1rdZ004.ken,gkn1rdZ008.ken,gkn1rdZ02.ken,gkn1rdZ05.kenMiller&ScaloIMF(forM£1,for110):kurZ0004.msc,kurZ004.msc,kurZ008.msc,kurZ02.msc,kurZ05.m
8、scKroupaIMF(forM£0.5,for0.51):imf27z0001.kro,imf27z0004.kro,imf27z004.kro,imf27z008.kro,imf27z02.kro,imf27z05.kro”