The active Algol binary KZ Pavonis
Budding, E., Marsden, S.C., and Slee, O.B. (2001) The active Algol binary KZ Pavonis. Publications of the Astronomical Society of Australia, 18 (2). pp. 140-147.
PDF (Published Version)
- Published Version
Restricted to Repository staff only
The Algol type eclipsing binary KZ Pav has been observed over one complete orbit (0.95 days) with theAustraliaTelescope CompactArray. Contemporaneous optical photometric data from the University of Southern Queensland's Observatory at Mount Kent were also collected and have been included in this multi-wavelength study.
Preliminary indications are that the low levels of emission observed share similarities to those of some RS CVn binaries. The optical data show phase-linked effects which can be related to the mass transfer process of Algols. The possibility that the radio emission may be related to this process is considered.
|Item Type:||Article (Refereed Research - C1)|
|Keywords:||stars: activity, stars: coronae, binaries: close, stars: individual (KZ Pavonis), radio continuum: stars, techniques: miscellaneou|
|Date Deposited:||14 Jul 2011 05:27|
|FoR Codes:||02 PHYSICAL SCIENCES > 0201 Astronomical and Space Sciences > 020110 Stellar Astronomy and Planetary Systems @ 100%|
|SEO Codes:||97 EXPANDING KNOWLEDGE > 970102 Expanding Knowledge in the Physical Sciences @ 100%|