Photometric Properties of Carbon Stars in the Small Magellanic Cloud

被引：0

作者：

Sloan, G. C. ^{[1
]}

Lagadec, E. ^{[2
]}

Kraemer, K. E. ^{[3
]}

Boyer, M. L. ^{[4
]}

Srinivasan, S. ^{[5
]}

McDonald, I. ^{[6
]}

Zijlstra, A. A. ^{[6
]}

机构：

[1] Cornell Univ, Ctr Radiophys & Space Res, Ithaca, NY 14853 USA

[2] Univ Nice Sophia Antipolis, Observ Cote Azur, Lab Lagrange, F-06189 Nice, France

[3] Boston Coll, Inst Sci Res, Chestnut Hill, MA 02167 USA

[4] NASA, Observat Cosmol Lab, Goddard Space Flight Ctr, Greenbelt, MD USA

[5] Taiwan Natl Univ, Acad Sinica, Inst Astron & Astrophys, Taipei, Taiwan

[6] Jodrell Bank Ctr Astrophys, Manchester, Lancs, England

来源：

WHY GALAXIES CARE ABOUT AGB STARS III: A CLOSER LOOK IN SPACE AND TIME | 2015年 / 497卷

关键词：

LONG-PERIOD VARIABLES; CATALOG;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Optical Gravitational Lensing Experiment identified over 1,800 carbon rich Mira and semi-regular variables in the Small Magellanic Cloud. Multi-epoch infrared photometry reveals that the semi-regulars and Miras follow different sequences in color-color space when using colors sensitive to molecular absorption bands. The dustiest Miras have the strongest pulsation amplitudes and longest periods. Efforts to determine bolometric magnitudes reveal possible systematic errors with published bolometric corrections.

引用

页码：429 / 434

页数：6

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