Please use this identifier to cite or link to this item: http://dspace.onu.edu.ua:8080/handle/123456789/4740
Title: About chemical composition of supergiant PMMR145 in Small Magellanic cloud. Osmium.
Authors: Gopka, Vera F.
Shavrina, Angelina V.
Vasilyeva, S. V.
Andrievsky, Serhii M.
Андрієвський, Сергій Михайлович
Андриевский, Сергей Михайлович
Citation: Odessa Astronomical Publications
Issue Date: 2012
Publisher: Astroprint
Keywords: Small Magellanic Cloud
star
evolution
supergiants
PMMR145
Series/Report no.: ;vol. 25, issue 2, p. 167-168.
Abstract: 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).
Description: Odessa Astronomical publications / Одесская астроном. обсерватория . – Одесса : Астропринт, 2012 . – Vol.25/2.
URI: http://dspace.onu.edu.ua:8080/handle/123456789/4740
Appears in Collections:Odessa Astronomical Publications

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