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On the determination of carbon isotopic ratios in cool carbon stars II. Accuracy of the iso-intensity method for crowded spectra
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Faculty of Science and Technology, Astronomical observatory.
1999 (English)In: ASTRONOMY AND ASTROPHYSICS, ISSN 0004-6361, Vol. 346, no 2, 520-522 p.Article in journal (Refereed) Published
Abstract [en]

de Laverny & Gustafsson (1998, Paper 1) questioned the iso-intensity method used by Ohnaka & Tsuji (1996) to derive carbon isotopic ratios in cool carbon stars. As a reply Ohnaka & Tsuji (1998) pointed out that the method criticized in Paper I differs fro

Place, publisher, year, edition, pages
SPRINGER VERLAG , 1999. Vol. 346, no 2, 520-522 p.
Keyword [en]
stars : abundances; stars : late-type; stars : AGB and post-AGB; stars : carbon; molecular processes; QUANTITATIVE-ANALYSIS
Identifiers
URN: urn:nbn:se:uu:diva-85277OAI: oai:DiVA.org:uu-85277DiVA: diva2:113185
Note
Addresses: de Laverny P, Observ Cote Azur, Dept Fresnel, UMR 6528, BP 4229, F-06304 Nice, France. Observ Cote Azur, Dept Fresnel, UMR 6528, F-06304 Nice, France. Astron Observ, S-75120 Uppsala, Sweden.Available from: 2008-10-17 Created: 2008-10-17 Last updated: 2011-01-14

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