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Subgiant CH stars. I. s-process abundances, C/O ratios, and evolutionary status
Document Type
Journal Article
Author
Source
Astrophys. J.; (United States); 259:2
Subject
71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS GIANT STARS
CHEMICAL COMPOSITION
HYDROCARBONS
ABUNDANCE
BARIUM
BINARY STARS
CARBON
CARBON STARS
DATA ANALYSIS
NUCLEOSYNTHESIS
OXYGEN
RED GIANT STARS
S PROCESS
STAR EVOLUTION
STRONTIUM
WHITE DWARF STARS
ALKALINE EARTH METALS
DWARF STARS
ELEMENTS
MAIN SEQUENCE STARS
METALS
NONMETALS
ORGANIC COMPOUNDS
STARS 640102* -- Astrophysics & Cosmology-- Stars & Quasi-Stellar, Radio & X-Ray Sources
Language
English
Abstract
Subgiant CH stars are late F to early G stars showing enhanced CH and Sr ii features on low-dispersion spectrograms. In this paper we report abundance analyses of seven relatively bright subgiant CH stars and the red-giant CH star HD 26, based on Palomar and Mount Wilson photographic coude spectrograms in the blue spectral region and on Mount Wilson coude scans in the red region.