Gopka, Vera F.Shavrina, Angelina V.Vasilyeva, S. V.Andrievsky, Serhii M.Андрієвський, Сергій МихайловичАндриевский, Сергей Михайлович2014-03-222014-03-222012Odessa Astronomical Publicationshttps://dspace.onu.edu.ua/handle/123456789/4740Odessa Astronomical publications / Одесская астроном. обсерватория . – Одесса : Астропринт, 2012 . – Vol.25/2.ABSTRACT. The abundance analysis of six Ksupergiants of the Small Magellanic (Hill 1997) showed that the heavier elements (La, Ce, Nd, Eu) have the excess relative to iron [El/Fe]=+0.4 dex, on average, for the sample of five stars (PMMR23, PMMR27, PMMR48, PMMR102, PMMR145). We made the identification of spectral lines in the spectrum of PMMR145 based on the comparison of synthetic and observed spectra. The absorption lines of elements heavier than lanthanides including osmium were identified and abundance of osmium was found ([Os/Fe]=0.59 dex).enSmall Magellanic CloudstarevolutionsupergiantsPMMR145Article