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An Improved uvby-Metallicity Calibration for Metal-rich Stars
We present an improved uvby-metallicity relation calibrated for F, G,and early K dwarfs and an analogous uvby-Teff relation, bothderived using a Levenberg-Marquardt minimization scheme. Ourcalibrations are based on 1533 stars that appear in both the Cayrel deStrobel metallicity compilation and in the Hauck-Mermilliod catalog ofuvby photometry. We also examine the speculative possibility of usinguvby photometry to produce a uvby-planeticity calibration. We concludethat while there is likely no strong photometric indicator of thepresence or absence of short-period planets, the possibility of aspectroscopic indicator of planeticity is well worth examining.
| Spectroscopic tests of photoelectric stellar classification of abnormal stars
Spectroscopic classification is obtained for 169 northern A5-G0 starspredicted by Olsen (1979, 1980) to have abnormal spectra on the basis ofStromgren four-color photometry. The success in identifying reddenedearly type stars was nearly 100 percent, for Am and early type weaklined stars about 75 percent, for stars above main sequence about 50percent, for composite spectra about 25 percent, and for Ap and LambdaBoo stars 0 percent. Thus photoelectric photometry is a successful firststep in discovering stars of the more extreme spectroscopicabnormalities.
| Estimation of spectral classifications for bright northern stars with interesting Stromgren indices
The purpose of this investigation is to provide spectroscopic observerswith finding lists of potentially interesting objects. From anunpublished UVBY catalogue of 7026 northern stars (mostly brighter than8.3m) 1094 objects with interesting combinations of UVBY indices havebeen selected. Most stars with post-HD classifications have beenexcluded, as well as late F dwarfs belonging to the intermediatepopulation II. For the 792 remaining stars estimated spectralclassifications are given. The techniques and experience from a previouspaper dealing with southern stars have been utilized here. Among thepredicted spectral classifications are 40 OB stars; 262 Ap, Am, or Fmstars; 16 supergiants of types A to G; 110 bright giants of types A to K(class II); 156 double stars or objects with composite spectra; 26 lateF dwarfs; 91 weak-lined dwarf and giant stars of types F to K, includingearly F-type population II field blue stragglers; and a few possiblefield horizontal branch stars, lambda Bootis-type stars, and late-typehalo giants.
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| Takýmyýldýz: | Koc |
| Sað Açýklýk: | 02h34m03.64s |
| Yükselim: | +12°10'51.1" |
| Görünürdeki Parlaklýk: | 7.497 |
| Uzaklýk: | 43.085 parsek |
| özdevim Sað Açýklýk: | 183.4 |
| özdevim Yükselim: | -34.6 |
| B-T magnitude: | 8.322 |
| V-T magnitude: | 7.566 |
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