The Active Algol Binary KZ Pavonis

E. Budding

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The Active Algol Binary KZ Pavonis

机译：活性Algol二进制KZ Pavonis

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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 Queenslanda€?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.

机译：使用澳大利亚望远镜紧凑型阵列在一个完整的轨道（0.95天）内观察到了Algol型日食双星KZ Pav。来自南昆士兰大学肯特山天文台的同时光学光度数据也已收集，并已包括在这项多波长研究中。初步迹象表明，观察到的低排放水平与某些RS CVn二进制文件具有相似之处。光学数据显示了相联效应，其可能与算法的传质过程有关。考虑了无线电发射可能与此过程有关的可能性。

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《Publications of the Astronomical Society of Australia》 |2013年第2期|共页
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E. Budding;
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The Active Algol Binary KZ Pavonis

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