Modeling of Debris Disks Resolved with Spitzer and HST

被引:0
|
作者
Stapelfeld, Karl R. [1 ]
Bryden, Geoffrey
Krist, John
Werner, Michael
Su, Kate
Rieke, George [2 ]
Watson, Dan [3 ]
Chen, Christine [4 ]
机构
[1] CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91125 USA
[2] Univ Arizona, Steward Observ, Tucson, AZ 85721 USA
[3] Univ Rochester, Rochester, NY 14627 USA
[4] Space Telescope Sci Inst, Baltimore, MD 21218 USA
关键词
circumstellar matter; DUST BELT; PLANET;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We summarize our ongoing effort to understand nearby debris disks through combined modeling of Spitzer MIPS imaging photometry, Spitzer IRS spectra, and HubbleSpaceTelescope scattered light images. A simple single-component model with minimum grain sizes equal to the blowout size works in two of four systems studied. Inner dust belts unseen by HST are required in two of four systems. The case of HD 10647 appears the most complex, where more than two dust belts may be needed.
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页码:43 / +
页数:2
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