Aug. 10, 13

   Tables of opacity due to bound-free absorption of C, N, O atoms. Compilation of TOPBASE data (Pavlenko Ya.V. & Zhukovska, S. 2002, KFNT, accepted). Read READ.ME in tared +gziped file...

   Grid of model atmospheres of Sakurai's object (2002, A&A, 390, 621).

   Grid of model atmospheres of carbon giants, 12C/13C=10. (Harris, G., Pavlenko, Ya, Jones, H.R.J, accepted by MNRAS, see astro-ph 0306141)

   Grid of model atmospheres of carbon giants, 12C/13C=3. (Harris, G., Pavlenko, Ya, Jones, H.R.J, accepted by MNRAS, see astro-ph 0306141)

   R CrB's 1D model atmospheres of different log N(Fe) (Pavlenko Ya.V. 1999. Astron. Rept, 43/2, pp. 94-103.)

   1D model atmosphere of Przybylski's star 6600/4.2 (Shavrina et al. 2003, AA, submitted)

   1D model atmospheres of the 4300/1.5 red giant (Arcturus). Abundances by Peterson et al. (1993, ApJ, 404, 333), but different log N(C) and log N(O), see Pavlenko (2007) submitted to Astron. Repts.

   Spectral regions contained of ''clean'' MgH features in the Arcturus spectrum.

   Molecular bands in spectra of M-stars.