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Near-infrared photometry of stars
Results are presented of infrared photometric observations performed oncomparison stars during a monitoring of long-period variables. Theseobservations, spread over a lapse of about 5 years, are used to derivethe J, H, and K magnitudes of 54 stars in the photometric systemdescribed by Koornneef (1983). The 1950.0 coordinates, spectral types,visual magnitudes, average magnitudes, and the number of observationsare given for each object.
| Scanner Abundance Studies. I. an Investigation of Supermetallicity in Late-Type Evolved Stars
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1969ApJ...157.1279S&db_key=AST
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| Сазвежђа: | Рибе |
| Ректацензија: | 01h05m09.15s |
| Deклинација: | +11°40'41.3" |
| Apparent магнитуда: | 8.423 |
| Proper motion RA: | 3.8 |
| Proper motion Dec: | -18.6 |
| B-T magnitude: | 10.06 |
| V-T magnitude: | 8.559 |
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