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Photometric Study of RX Cephei
Photoelectric observations of RX Cephei from Zsoldas and McAdam (1993)and the authors, and long term visual observations from Schmude and theAAVSO were analyzed. RX Cep, whose variability has been questioned,appears to have become 0.15 magnitude brighter between 1990 and 2000.There is also some evidence of a 350-day period. The B-V color index ofthis star may also be calculated as 1.12+/-0.04.
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Not Available
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Osservazione e dati astrometrici
| Costellazione: | Cefeo |
| Ascensione retta: | 01h40m31.63s |
| Declinazione: | +81°25'47.4" |
| Magnitudine apparente: | 7.131 |
| Distanza: | 299.401 parsec |
| Moto proprio RA: | -8.5 |
| Moto proprio Dec: | -1.2 |
| B-T magnitude: | 7.11 |
| V-T magnitude: | 7.13 |
Cataloghi e designazioni:
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INHABITED SKY
