Publication Abstracts
Oinas 1974
Oinas, V., 1974: Strong-line K stars. I. Photometry. Astrophys. J. Supp. Series, 27, 391-404, doi:10.1086/190302.
Absolute spectrophotometric photometry has been performed for 26 super-metal-rich (SMR) and normal giants and dwarfs of spectral type K. Emergent fluxes from model atmospheres in conjunction with blanketing corrections derived from high-dispersion spectra are used to obtain effective temperatures. Hα wing strengths are also discussed in relation to temperatures and metal abundances, and the material is used to construct an H-R diagram for the program stars. The positions of the SMR dwarfs on the main sequence as well as the Hα strengths lend support to the conclusion that these stars are metal rich to a moderate degree. The excess blanketing in the SMR stars is shown to have only a small effect on the emergent flux.
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BibTeX Citation
@article{oi06000g,
author={Oinas, V.},
title={Strong-line K stars. I. Photometry},
year={1974},
journal={Astrophys. J. Supp. Series},
volume={27},
pages={391--404},
doi={10.1086/190302},
}
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RIS Citation
TY - JOUR ID - oi06000g AU - Oinas, V. PY - 1974 TI - Strong-line K stars. I. Photometry JA - Astrophys. J. Supp. Series VL - 27 SP - 391 EP - 404 DO - 10.1086/190302 ER -
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