TX Cancri, the golden wonder

TX Cancri, the golden wonder
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DOI:
10.1086/152215
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发表时间:
1973-07
期刊:
The Astrophysical Journal
影响因子:
--
通讯作者:
J. Whelan;S. P. Worden;S. Mochnacki
J. Whelan;S. P. Worden;S. Mochnacki
中科院分区:
其他
文献类型:
--
作者:
J. Whelan;S. P. Worden;S. Mochnacki

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本文报道了位于Praesepe的WUMa型双星系统TX Cancri的分光、光度和偏振观测结果。确定了系统各组成部分的参数(质量、半径、光度)。如果系统是演化的,那么它必须有足够的质量才能达到目前的状态。我们认为,TX Cnc是未进化的,零年龄接触的二元模型的系统构造。讨论了系统参数和零龄模型的解释问题。
Spectrososopic, photometric, and polarimetric observations of TX Cancri, a W UMa-type binary system in Praesepe, are reported. The parameters (masses, radii, luminosities) of the components of the system are determined. If the system is evolved, then it must have last a substantial amount of mass to reach its present state. We argue that TX Cnc is unevolved, and an age-zero contact- binary model for the system is constructed. Problems in the interpretation of the parameters of the system and the age-zero model are discussed.