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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
| The catalogue of nearby stars metallicities. Not Available
| Optical Polarization of 1000 Stars Within 50-PARSECS from the Sun Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1993A&AS..101..551L&db_key=AST
| Predicted infrared brightness of stars within 25 parsecs of the sun Procedures are given for transforming selected optical data intoinfrared flux densities or irradiances. The results provide R, T(eff)blackbody approximations for about 2000 of the stars in Woolley et al.'sCatalog of Stars (1970) within 25 pc of the sun, and additional whitedwarfs, with infrared flux densities predicted for them at ninewavelengths from 2.2 to 101 microns including the Infrared AstronomySatellite bands.
| Optical polarization of stars of galactic latitudes b-45 degres. Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1976A&AS...23..125S&db_key=AST
| UBV Photometry of 500 Southern Stars [erratum: 1973MNSSA..32...48C] Not Available
| Standard magnitudes in the E regions. Not Available
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Сазвежђа: | Феникс |
Ректацензија: | 01h14m25.06s |
Deклинација: | -41°53'39.2" |
Apparent магнитуда: | 8.467 |
Даљина: | 135.135 parsecs |
Proper motion RA: | -108.8 |
Proper motion Dec: | -54.5 |
B-T magnitude: | 9.135 |
V-T magnitude: | 8.523 |
Каталог и designations:
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