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On the determination of carbon isotopic ratios in cool carbon stars
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Faculty of Science and Technology, Astronomical observatory.
1998 (English)In: ASTRONOMY AND ASTROPHYSICS, ISSN 0004-6361, Vol. 332, no 2, 661-671 p.Article in journal (Refereed) Published
Abstract [en]

We discuss the determination of carbon isotopic ratios C-12/C-13 in N-type Galactic carbon stars. Ohnaka & Tsuji (1996) reported C-12/C-13 ratios Smaller by a factor 2 or 3 than the determinations of Lambert et al. (1986). Using synthetic spectra of carbo

Place, publisher, year, edition, pages
SPRINGER VERLAG , 1998. Vol. 332, no 2, 661-671 p.
Keyword [en]
stars : abundances; stars : AGB and post-AGB; stars : carbon; molecular processes; LUNAR OCCULTATION TECHNIQUE; ANGULAR DIAMETERS; CHEMICAL-COMPOSITION; ASTROPHYSICAL INTEREST; DISSOCIATION-ENERGY; EVOLVED STARS; GALACTIC DISK; GIANT BRANCH; TX-PISCIUM; R
Identifiers
URN: urn:nbn:se:uu:diva-85318OAI: oai:DiVA.org:uu-85318DiVA: diva2:113226
Note
Addresses: de Laverny P, Astron Observ, Box 515, S-75120 Uppsala, Sweden. Astron Observ, S-75120 Uppsala, Sweden.Available from: 2008-10-17 Created: 2008-10-17 Last updated: 2011-01-14

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