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Derivation of the Galactic rotation curve using space velocities
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This paper investigates the degree of success with which uvby photometrycan be applied to predict spectral classifications for 947 A, F, and Gstars brighter than an apparent magnitude of 8.3 and with four-colorindices indicating some kind of interesting, unusual, or peculiarspectrum. One or several possible spectral classifications are estimatedfor each star from photometry alone, double stars are distinguished, andthe estimates are compared with published classifications. The resultsshow that the framework provided by uvby photometry can be extended toinclude most G and K stars, reddened stars, peculiar stars, and certaintypes of double star.
| Multicolor photometry of metallic-line stars. III. A photometric catalogue
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1974RMxAA...1..175M&db_key=AST
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Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1974AJ.....79.1290F&db_key=AST
| Catalogue et bibliographie des étoiles A à spectre particulier - Deuxième supplément
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Osservazione e dati astrometrici
| Costellazione: | Poppa |
| Ascensione retta: | 08h08m00.34s |
| Declinazione: | -35°12'39.8" |
| Magnitudine apparente: | 7.193 |
| Distanza: | 147.275 parsec |
| Moto proprio RA: | 3.4 |
| Moto proprio Dec: | -6.2 |
| B-T magnitude: | 7.629 |
| V-T magnitude: | 7.229 |
Cataloghi e designazioni:
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INHABITED SKY
