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Contribution to the search for binaries among Am stars - V. Orbital elements of eight short-period spectroscopic binaries
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The Glazar telescope, installed on the Kvant module of the Mir spacestation, started regular observations in August 1987. This paperpresents results of the photometry of 15 stars detected by the Glazartelescope at 1640 A in an area of about 28 sq deg at high Galacticlongitudes.
| 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
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Observation and Astrometry data
| Constellation: | アンドロメダ座 |
| Right ascension: | 00h08m09.60s |
| Declination: | +31°22'44.4" |
| Apparent magnitude: | 7.254 |
| Distance: | 204.082 parsecs |
| Proper motion RA: | 45.2 |
| Proper motion Dec: | -2.9 |
| B-T magnitude: | 7.5 |
| V-T magnitude: | 7.275 |
Catalogs and designations:
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