Model atmosphere of Hauschildt et al (1999), 
solar abundances, (K14) labels the data from R.Kurucz's web page, i.e 
kurucz.harvard.edu. 


ng.28-5.0-0.0.TiO_alpha_3.fl.v    <-- Alpha
ng.28-5.0-0.0.TiO_beta.fl.v       <-- beta
ng.28-5.0-0.0.TiO_delta.fl.v      <-- delta
ng.28-5.0-0.0.TiO_eps_3.fl.v      <-- epsilon
ng.28-5.0-0.0.TiO_gamma_3.fl.v    <-- gamma
ng.28-5.0-0.0.TiO.gammap3.fl.v    <-- gamma prim
ng.28-5.0-0.0.TiO_phi.fl.v        <-- phi



ng.28-5.0-0.0.alo.v       <-- AlO B-X
ng.28-5.0-0.0.cah.ax.v    <-- CaH A-X
ng.28-5.0-0.0.CaH.BX.fl.v <-- CaH B-X
ng.28-5.0-0.0.cah.bx.v    <-- 
ng.28-5.0-0.0.cnb.v       <-- CN (blue)
ng.28-5.0-0.0.cnr.v       <-- CN (red)
ng.28-5.0-0.0.CrH.AX.fl.v <-- CrH (A-H)
ng.28-5.0-0.0.feh.3k      <-- FeH (A-X)
ng.28-5.0-0.0.h2o.3k      <-- H2O
ng.28-5.0-0.0.mgh.v       <-- MgH(A-H) 
ng.28-5.0-0.0.VO_A-X.fl.v <-- VO (A-H)
ng.28-5.0-0.0.VO_B-X.fl.v <-- VO (B-H)