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Contributions to the Nearby Stars (NStars) Project: Spectroscopy of Stars Earlier than M0 within 40 pc-The Southern Sample We are obtaining spectra, spectral types, and basic physical parametersfor the nearly 3600 dwarf and giant stars earlier than M0 in theHipparcos catalog within 40 pc of the Sun. Here we report on resultsfor 1676 stars in the southern hemisphere observed at Cerro TololoInter-American Observatory and Steward Observatory. These resultsinclude new, precise, homogeneous spectral types, basic physicalparameters (including the effective temperature, surface gravity, andmetallicity [M/H]), and measures of the chromospheric activity of ourprogram stars. We include notes on astrophysically interesting stars inthis sample, the metallicity distribution of the solar neighborhood, anda table of solar analogs. We also demonstrate that the bimodal nature ofthe distribution of the chromospheric activity parameterlogR'HK depends strongly on the metallicity, andwe explore the nature of the ``low-metallicity'' chromosphericallyactive K-type dwarfs.
| The general catalogue of trigonometric [stellar] paralaxes Not Available
| Erratum - Errors or Omissions in Star-Identifications in the General Catalogue of Trigonometric Stellar Parallaxes Not Available
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Gözlemler ve gökölçümü verileri
Takýmyýldýz: | Karina |
Sað Açýklýk: | 10h26m47.56s |
Yükselim: | -62°54'09.4" |
Görünürdeki Parlaklýk: | 9.911 |
Uzaklýk: | 27.049 parsek |
özdevim Sað Açýklýk: | -273.7 |
özdevim Yükselim: | -370.1 |
B-T magnitude: | 11.209 |
V-T magnitude: | 10.019 |
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