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New Photoelectric Light Curves of AB Andromedae
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| Photoelectric observations of W UMa stars - U Pegasi and AB Andromedae
The quadratic ephemerides of the W UMa systems U Pegasi and ABAndromedae are computed from photoelectric and photometric data toanalyze the objects' periodicities. The minima obtained for the presentwork are incorporated into the minima obtained by Lafta and Grainger(1986) for the quadratic ephemerides calculation. U Pegasi is found tohave a decreasing period with a rate of change of -0.91 s/century, whileAB Andromedae increases steadily at 0.83 s/century, and the existence ofa third unseen object is postulated.
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Member of following groups:
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Observation and Astrometry data
| Constellation: | Andromeda |
| Right ascension: | 23h11m39.59s |
| Declination: | +36°47'40.7" |
| Apparent magnitude: | 8.327 |
| Distance: | 6666.667 parsecs |
| Proper motion RA: | 0 |
| Proper motion Dec: | -26.1 |
| B-T magnitude: | 9.585 |
| V-T magnitude: | 8.431 |
Catalogs and designations:
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