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uvby - β Photoelectric Photometry of the Open Cluster α Per
Absolute photoelectric photometry of stars in the direction of the OpenCluster α Per has been secured and is presented along with ananalysis reinforced with all the available data in Strömgrenuvby-β photometry compiled from the literature. Cluster membershipis analyzed and the physical characteristics of the stars have beendeduced. The membership determined in this paper is compared with thatof proper motion studies and Hipparcos.
| Eigenbewegungen in der Umgebung von α Persei
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Member of following groups:
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Observation and Astrometry data
| Constellation: | Persée |
| Right ascension: | 03h26m04.47s |
| Declination: | +49°44'44.1" |
| Apparent magnitude: | 7.124 |
| Distance: | 1388.889 parsecs |
| Proper motion RA: | 4 |
| Proper motion Dec: | 1.7 |
| B-T magnitude: | 7.557 |
| V-T magnitude: | 7.16 |
Catalogs and designations:
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INHABITED SKY
