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The atmosphere of the peculiar binary system ET Andromedae
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Astronomy and Space Physics.
1995 (English)In: Astronomy & Astrophysics, ISSN 0004-6361, Vol. 294, no 3, 757- p.Article in journal (Refereed) Published
Abstract [en]

High spectral resolution, high signal-to-noise OHP spectra which cover the range from 4000A to 7500A were used to derive abundances for ET And. An extreme overabundance of silicon by nearly 100 times of the solar value corroborates the Si-star classificat

Place, publisher, year, edition, pages
EDP Sciences , 1995. Vol. 294, no 3, 757- p.
Keyword [en]
ABUNDANCE, BINARY STARS, PECULIAR STARS, RARE EARTH ELEMENTS, SILICON, STELLAR ATMOSPHERES, STELLAR COMPOSITION, LINE SPECTRA, MAIN SEQUENCE STARS, SPECTRAL RESOLUTION, STELLAR EVOLUTION
Identifiers
URN: urn:nbn:se:uu:diva-41297OAI: oai:DiVA.org:uu-41297DiVA: diva2:69198
Available from: 2008-10-17 Created: 2008-10-17 Last updated: 2011-01-16

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