Variable stars in the Magellanic Clouds -: II.: The data and infrared properties

被引：65

作者：

Ita, Y ^{[1
]}

Tanabé, T

Matsunaga, N

Nakajima, Y

Nagashima, C

Nagayama, T

Kato, D

Kurita, M

Nagata, T

Sato, S

Tamura, M

Nakaya, H

Nakada, Y

机构：

[1] Univ Tokyo, Sch Sci, Inst Astron, Tokyo 1810015, Japan

[2] Japan Aerosp Explorat Agcy, Inst Space & Astronaut Sci, Kanagawa 2298510, Japan

[3] Natl Astron Observ Japan, Tokyo 1818588, Japan

[4] Nagoya Univ, Dept Astrophys, Chikusa Ku, Nagoya, Aichi 4648602, Japan

[5] Natl Astron Observ Japan, Subaru Telescope, Hilo, HI 96720 USA

[6] Univ Tokyo, Sch Sci, Kiso Observ, Nagano 3970101, Japan

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2004年 / 353卷 / 03期

关键词：

surveys; stars : AGB and post-AGB; stars : variables : other; Magellanic Clouds; galaxies : stellar content; infrared : stars;

D O I：

10.1111/j.1365-2966.2004.08126.x

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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.

引用

页码：705 / 712

页数：8

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