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Spectral Classification of Stars in A Supplement to the Bright Star Catalogue
MK spectral types are given for about 584 stars in A Supplement to theBright Star Catalogue. These are compared with Hipparcos parallaxes tocheck the reliability of those classifications. The estimated errors are+/-1.2 subtypes, and 10% of the luminosity classes may be wrong.
| Vitesses radiales. Catalogue WEB: Wilson Evans Batten. Subtittle: Radial velocities: The Wilson-Evans-Batten catalogue.
We give a common version of the two catalogues of Mean Radial Velocitiesby Wilson (1963) and Evans (1978) to which we have added the catalogueof spectroscopic binary systems (Batten et al. 1989). For each star,when possible, we give: 1) an acronym to enter SIMBAD (Set ofIdentifications Measurements and Bibliography for Astronomical Data) ofthe CDS (Centre de Donnees Astronomiques de Strasbourg). 2) the numberHIC of the HIPPARCOS catalogue (Turon 1992). 3) the CCDM number(Catalogue des Composantes des etoiles Doubles et Multiples) byDommanget & Nys (1994). For the cluster stars, a precise study hasbeen done, on the identificator numbers. Numerous remarks point out theproblems we have had to deal with.
| UBV Photoelectric Photometry Catalogue (1986). III Errors and Problems on DM and HD Stars
Not Available
| Photometric UBV period study of eight AP stars
Eight Ap stars for which periods had been determined by Winzer (1974)were the subject of an independent period determination. All were starswhich were found to be short-period variables and which showed thetypical small-amplitude variation associated with short periods. For sixof these, the period was confirmed. For one, HR 9017, a different andbetter period was determined and for the remaining star, HR 4430,periodic variation was not observed.
| Visual multiples. VII - MK classifications
Classifications are given for 865 components of visual multiples; theyshow no systematic differences from the MK system, and the random errorsare one subclass in type and two-thirds of a luminosity class. It isfound that at least 1% of the F-type IV and V stars are weak-lined, 32%of the A4-F1 IV and V stars are Am, and 5% of the A0-A3 IV and V starsare early-type Am. Attention is called to the large fraction (55%) ofthe A3-A9 III-V stars that are of luminosity classes III or IV, unlikethe percentage (16%) at neighboring types.
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| Takýmyýldýz: | Calgi |
| Sað Açýklýk: | 19h09m23.13s |
| Yükselim: | +30°33'58.6" |
| Görünürdeki Parlaklýk: | 6.924 |
| Uzaklýk: | 452.489 parsek |
| özdevim Sað Açýklýk: | -4.6 |
| özdevim Yükselim: | -0.8 |
| B-T magnitude: | 6.83 |
| V-T magnitude: | 6.917 |
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