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GCVS Variability Types and Distribution Statistics of Designated Variable Stars According to their Types of Variability ======================================================================== I. GCVS Variability Types. ... The new variability types (ZZO, AM, R, BE, LBV, BLBOO) have been added in the Name-Lists 67- 72 and in the GCVS vol.V. ZZO ZZ Cet type variables of the DO spectral type showing HeII and and CIV absorbtion lines in their spectra. ... RCB Variables of the R Coronae Borealis type. ...

... The spectrum of the brightest star, our Sun, shows several dark gaps perpendicular to the flow of it’s colours (figure 1). These so called spectral absorption lines where discovered in 1802 by the English scientist William Wollaston. ... Some stars as Pollux show a spectrum similar to that of our sun with strong Ca II and Fe II lines, others as Sirius or Vega show strong absorption lines of hydrogen, others, as Mira show very complicated spectra due to molecular absorption lines (see figure 5). ...

Stochastic Models of Hot Planetary and Satellite Coronas . ... Shematovich, V.I., Bisikalo , D.V., and Gerard, J.-C. Nonequilibrium Processes in the Planetary and Cometary Atmospheres: Theory and Applications , Dordrecht : Kluwer Academic, 1997. ... Res. ... Shematovich, V.I., Bisikalo , D.V., and Gerard, J.-C. A Kinetic Model of the Formation of the Hot Oxygen Geocorona . ... Shematovich, V.I., Bisikalo , D.V., and Gerard, J.-C. A kinetic model of the formation of the hot oxygen geocorona . ...

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