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Abundance analysis of roAp stars - V. HD 166473
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Astronomy and Space Physics.
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2000 (English)In: ASTRONOMY AND ASTROPHYSICS, ISSN 0004-6361, Vol. 356, no 1, 200-208 p.Article in journal (Refereed) Published
Abstract [en]

This fifth paper in a sequence on abundance analyses of roAp stars features several improvements and complements over the previous investigations: i. The new VALD-2 atomic data base was used which significantly improves the analysis of C, N, O, and rare e

Place, publisher, year, edition, pages
SPRINGER VERLAG , 2000. Vol. 356, no 1, 200-208 p.
Keyword [en]
stars : abundances; stars : atmospheres; stars : chemically peculiar; stars : fundamental parameters; stars : individual : HD166473; ATOMIC-TRANSITION-PROBABILITIES; I OSCILLATOR-STRENGTHS; AP STARS; FE-I; SOLAR ABUNDANCE; LIFETIMES; ENERGIES; LUTETIUM; L
URN: urn:nbn:se:uu:diva-36635OAI: oai:DiVA.org:uu-36635DiVA: diva2:64534
Addresses: Weiss WW, Univ Vienna, Inst Astron, Turkenschanzstr 17, A-1180 Vienna, Austria. Univ Vienna, Inst Astron, A-1180 Vienna, Austria. Russian Acad Sci, Astron Inst, Moscow 109017, Russia. Astron Observ, S-75120 Uppsala, Sweden. European So Observ,Available from: 2008-10-17 Created: 2008-10-17 Last updated: 2011-01-14

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