6533b85afe1ef96bd12b8b0f
RESEARCH PRODUCT
The chemical composition of extremely metal-poor and carbon-rich star HD 112869
L. ZacsO. AlksnisI. Diebelesubject
Materials scienceK-type main-sequence starMetallicitychemistry.chemical_elementAstronomyAstronomy and AstrophysicsAstrophysicsCarbon starRadial velocityAtmosphereT Tauri starchemistrySpace and Planetary ScienceCarbonO-type main-sequence stardescription
The preliminary results of abundance analysis are presented for extremely metal-poor carbon star HD 112869 = TT CVn = CGCS 3319. The radial velocity was found to be −137.7 km s −1 . Our LTE abundance analysis supports an extremely low metallicity for TT CVn, [Fe/H] = −3.2, and a significant overabundance of carbon and neutron-capture elements. The 12 C/ 13 C ratio in the atmosphere of HD 112869 is high.
| year | journal | country | edition | language |
|---|---|---|---|---|
| 2005-05-01 | Proceedings of the International Astronomical Union |