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NP Pavonis : Differential Corrections Analysis of the UBV Observations
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| The Active Algol Binary KZ Pavonis
The Algol type eclipsing binary KZ Pav has been observed over onecomplete orbit (0.95 days) with theAustralia Telescope CompactArray.Contemporaneous optical photometric data from the University of SouthernQueensland's Observatory at Mount Kent were also collected and have beenincluded in this multi-wavelength study. Preliminary indications arethat the low levels of emission observed share similarities to those ofsome RS CVn binaries. The optical data show phase-linked effects whichcan be related to the mass transfer process of Algols. The possibilitythat the radio emission may be related to this process is considered.
| First Determinations of Photoelectric Minima, Real Period and Study of the Period of NP Pav
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| The eclipsing binary system KZ Pav
Not Available
| Behavior of the CA II-K line in the cool AP star HD 197417
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Osservazione e dati astrometrici
| Costellazione: | Pavone |
| Ascensione retta: | 20h58m11.68s |
| Declinazione: | -69°08'46.4" |
| Magnitudine apparente: | 6.831 |
| Distanza: | 165.837 parsec |
| Moto proprio RA: | 15.8 |
| Moto proprio Dec: | -29.5 |
| B-T magnitude: | 6.767 |
| V-T magnitude: | 6.826 |
Cataloghi e designazioni:
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