Published April 15, 1982
| Version v1
Journal article
K giant with an unusually high abundance of lithium: HD 112127
Creators
- 1. Joint Institute for Laboratory Astrophysics, University of Colorado and National Bureau of Standards
Description
The strong-lined K giant star HD 112127 exhibits an extremely strong lithium resonance line in its spectrum. In most other respects the atmosphere of the star resembles the well-studied, strong-lined star μ Leo. A model atmosphere analysis has been carried out for HD 112127 with particular emphasis on the light element abundances. Iron peak elements show essentially solar composition while the CNO group is enhanced by about 0.2 dex. The carbon isotope ratio is near 20, while the lithium content of this star is approximately the maximum seen in unevolved stars. Schemes for the production of lithium in a relatively low luminosity giant are discussed
Additional details
Publishing Information
- Journal Title
- Astrophys. J.
- Journal Volume
- 255
- Journal Issue
- 2
- Series
- Astrophys. J.
- Journal Page Range
- 577-584
- ISSN
- 0004-637X
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 14730351
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- CARBON 12; CARBON 13; CHEMICAL COMPOSITION; GIANT STARS; ISOTOPE RATIO; LITHIUM; NITROGEN; OXYGEN; SPECTRA; STAR MODELS; STELLAR ATMOSPHERES
- Descriptors DEC
- ALKALI METALS; ATMOSPHERES; CARBON ISOTOPES; ELEMENTS; EVEN-EVEN NUCLEI; EVEN-ODD NUCLEI; ISOTOPES; LIGHT NUCLEI; MATHEMATICAL MODELS; METALS; NONMETALS; NUCLEI; STABLE ISOTOPES; STARS