Variable stars in the Magellanic Clouds – II. The data and infrared properties
Variable stars in the Magellanic Clouds – II. The data and infrared properties
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DOI：
10.1111/j.1365-2966.2004.08126.x
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发表时间：
2003-12
影响因子：
4.8
通讯作者：
Y. Ita;T. Tanabé;N. Matsunaga;Y. Nakajima;C. Nagashima;T. Nagayama;D. Kato;M. Kurita;T. Nagata;S. Sato;M. Tamura;H. Nakaya;Yoshikazu Nakada University of Tokyo Naoj Nagoya University Subaru-Yoshikazu-Nakada-University-of-Tokyo-Naoj-Nagoya-102835465;Naoj Kiso Observatory Jaxa
中科院分区：
文献类型：
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作者：
Y. Ita;T. Tanabé;N. Matsunaga;Y. Nakajima;C. Nagashima;T. Nagayama;D. Kato;M. Kurita;T. Nagata;S. Sato;M. Tamura;H. Nakaya;Yoshikazu Nakada University of Tokyo Naoj Nagoya University Subaru-Yoshikazu-Nakada-University-of-Tokyo-Naoj-Nagoya-102835465;Naoj Kiso Observatory Jaxa
本文介绍了OGLE巡天在大麦哲伦云和小麦哲伦云中分别探测到的8852颗和2927颗变星的资料。它们与SIRIUS JHK巡天数据进行了交叉识别，并讨论了它们的红外特性。变星红巨星在周期-（J-K）平面上的分离很好，这表明周期-（J-K）平面是区分其脉动方式和类型的一个很好的工具。
The data of 8852 and 2927 variable stars detected by the OGLE survey in the Large and Small Magellanic Clouds are presented. They are cross-identified with the SIRIUS JHK survey data, and their infrared properties are discussed. Variable red giants are well separated on the period-(J - K) plane, suggesting that it could be a good tool to distinguish their pulsation mode and type.