Spitzer/IRAC observations of AGB stars

被引：0

作者：

Marengo, Massimo ^{[1
]}

Reiter, Megan ^{[2
]}

Fazio, Giovanni G. ^{[1
]}

机构：

[1] Harvard Smithsonian Ctr Astrophys, Cambridge, England

[2] Univ Calif Berkeley, Berkeley, CA 94720 USA

来源：

NINTH TORINO WORKSHOP ON EVOLUTION AND NUCLEOSYNTHESIS IN AGB STARS AND THE SECOND PERUGIA WORKSHOP ON NUCLEAR ASTROPHYSICS | 2008年

基金：

美国国家科学基金会;

关键词：

infrared : stars; stars : AGB and post-AGB; carbon; mass loss; variables : other;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present here the first observation of galactic AGB stars with the InfraRed Array Camera (IRAC) onboard the Spitzer Space Telescope. Our sample consists of 48 AGB stars of different chemical signature, mass loss rate and variability class. For each star we have measured IRAC photometry and colors, Preliminary results shows that IRAC colors are sensitive to spectroscopic features associated to molecules and dust in the AGB wind. Period is only loosely correlated to the brightness of the stars in the IRAC bands. We do find, however, a tight period-color relation for sources classified as "semiregular" variables. This may be interpreted as the lack of warm dust in the wind of the sources in this class, as opposed to Mira variables that show higher infrared excess in all IRAC bands.

引用

页码：331 / +

页数：2

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