The chemical composition of IRAS 05341+0852: a post-AGB F supergiant with 21 μm emission
نویسندگان
چکیده
منابع مشابه
The chemical composition of IRAS 05341+0852: a post-AGB F supergiant with 21μm emission
An abundance analysis of the photosphere of the F-type Post-AGB candidate IRAS 05341+0852 is presented. The analysis of the spectra suggests that the atmospheric model: Teff=6500 K, log g=0.5, ξt=5 km s−1 and [M/H]=1.0, best represents the photosphere of the star. We find that the star is metal-poor ([Fe/H]=−0.9) and carbon-rich (C/O≈1.9). Lithium, carbon, nitrogen, oxygen, aluminum and silicon...
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ژورنال
عنوان ژورنال: Symposium - International Astronomical Union
سال: 1997
ISSN: 0074-1809
DOI: 10.1017/s0074180900131419