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Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS) - Third edition - Comments and statistics
The Catalogue, available at the Centre de Données Stellaires deStrasbourg, consists of 13 573 records concerning the results obtainedfrom different methods for 7778 stars, reported in the literature. Thefollowing data are listed for each star: identifications, apparentmagnitude, spectral type, apparent diameter in arcsec, absolute radiusin solar units, method of determination, reference, remarks. Commentsand statistics obtained from CADARS are given. The Catalogue isavailable in electronic form at the CDS via anonymous ftp tocdsarc.u-strasbg.fr (130.79.128.5) or viahttp://cdsweb.u-strasbg.fr/cgi-bin/qcar?J/A+A/367/521
| 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.
| The detection of close binary systems in observations of lunar occultations with a 6-m telescope
The paper presents the results of photoelectric observations of thelunar occultation of 10 stars which were carried out with the 6-mtelescope of the Special Astrophysical Observatory of the USSR Academyof Sciences. The brightness strip distribution of the occulted source isrestored using a modified regularization method in which a prioriinformation on the nonnegativity of the solution is accounted for. Theupper limits to the angular diameters of eight stars are obtained. For astar with a brightness of 11.07 mag, an angular resolution of 0.0101 isachieved. The following close binary systems were detected: SAO 128720and SAO 110268.
| Intermediate band, H-beta, and RI photometry of a large sample of stars unbiased with respect to their motion. I - The F-type stars
Intermediate band and H-beta data from a sample of 1000 stars earlierthan type G2 are presented and discussed relative to the stars'luminosities, metal abundances, and motion. Two groups of stars areconsidered, one within 10 arcsec of the South Galactic Pole and 8.5-8.6mag stars contained in the Moore-Paddock (1950) and Wayman (1960)samples (MP-W). The MP-W stars are mainly old disk population stars withmetal abundances of 4-0.25 solar values. Possible age-abundancedistribution-luminosity connections are explored, as are techniques forseparating old and young disk population objects.
| Observations of Lunar Occultations of Stars with the 6-METER Telescope
Not Available
| Radial Velocities, Spectral Types, and Luminosity Classes of 820 Stars.
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1950ApJ...112...48M&db_key=AST
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Osservazione e dati astrometrici
| Costellazione: | Pesci |
| Ascensione retta: | 01h58m56.48s |
| Declinazione: | +06°40'26.7" |
| Magnitudine apparente: | 8.406 |
| Distanza: | 151.745 parsec |
| Moto proprio RA: | 29.6 |
| Moto proprio Dec: | -12.3 |
| B-T magnitude: | 8.819 |
| V-T magnitude: | 8.441 |
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