Mineralogy of circumstellar dust

被引：0
|
作者：
Waters, L. B. F. M. [1 ,2 ]
Leinert, Ch. [3 ]
机构：
[1] Univ Amsterdam, Astron Inst Anton Pannekoek, Kruislaan 403, NL-1098 SJ Amsterdam, Netherlands
[2] Katholieke Univ Leuven, Inst Sterrenkunde, Leuven, Belgium
[3] Max Planck Inst Astronomie, Heidelberg D-69117, Germany
来源：
POWER OF OPTICAL/IR INTERFEROMETRY: RECENT SCIENTIFIC RESULTS AND 2ND GENERATION INSTRUMENTATION | 2008年
关键词：
D O I：
10.1007/978-3-540-74256-2_18
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The composition and spatial distribution of circumstellar dust in young and old stars can be used as a probe of the physical and chemical processes that take place. Such studies require a modest spectral resolution in combination with high spatial resolution and large collecting area, now for the first time provided by the new generation of optical interferometers. This review discusses some early results from the VLT Interferometer in the area of circumstellar dust.
引用
收藏
页码：163 / 173
页数：11
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