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Chemical abundances in cool metal rich disk dwarf stars
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Astronomy and Space Physics.
2000 (English)In: ASTRONOMY AND ASTROPHYSICS, ISSN 0004-6361, Vol. 363, no 2, 692-704 p.Article in journal (Refereed) Published
Abstract [en]

The present study of spectra of twelve metal-rich cool dwarf stars, carefully selected in order to cover a range of temperatures (similar to 4400 - 6000 K), is a follow UP On Feltzing & Gustafsson (1998) with the aim to understand the apparent over-ioniza

Place, publisher, year, edition, pages
SPRINGER-VERLAG , 2000. Vol. 363, no 2, 692-704 p.
Keyword [en]
stars : late-type; stars : abundances; NEUTRAL HYDROGEN-ATOMS; MODEL ATMOSPHERES; UVBY PHOTOMETRY; GALACTIC DISK; NON-LTE; TRANSITIONS; CALCIUM; COLLISIONS; EVOLUTION; BRIGHTER
Identifiers
URN: urn:nbn:se:uu:diva-36667OAI: oai:DiVA.org:uu-36667DiVA: diva2:64566
Note
Addresses: Thoren P, Uppsala Astron Observ, Box 515, S-75120 Uppsala, Sweden. Uppsala Astron Observ, S-75120 Uppsala, Sweden. Lund Observ, S-22100 Lund, Sweden.Available from: 2008-10-17 Created: 2008-10-17 Last updated: 2011-01-14

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