Please use this identifier to cite or link to this item: http://dspace.onu.edu.ua:8080/handle/123456789/4806
Title: CHEMICAL COMPOSITION OF PECULIAR STAR HD91375 THE MEMBER OF SIRIUS MOVING GROUP
Authors: Yushchenko, V. A.
Citation: Odessa Astronomical Publications
Issue Date: 2010
Publisher: Astroprint
Keywords: stars
abundances
individual (HD91375, Sirius)
Series/Report no.: ;vol. 22, p. 73-76
Abstract: We present the results of determinations of the abundances of chemical elements in the atmosphere of hot chemically peculiar star HD91375 - member of Sirius moving group. We used the observations made at 8.2 meter ESO telescope. The abundance pattern of HD91375 is found for the first time, the comparison with the abundances of Sirius A is made. The abundance patterns of Sirius and HD91375 are clearly different. It confirms the possibility of recent accretion event in the Sirius binary system.
Description: Odessa Astronomical publications / Одесская астроном. обсерватория . – Одесса : Астропринт, 2009/2010 . – Vol.22.
URI: http://dspace.onu.edu.ua:8080/handle/123456789/4806
Appears in Collections:Odessa Astronomical Publications

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