The VLTI and its instrumentation

被引：0
|
作者：
Richichi, A [1 ]
Glindemann, A [1 ]
Schöller, M [1 ]
机构：
[1] European So Observ, D-85748 Garching, Germany
来源：
ORIGINS OF STARS AND PLANETS: THE VLT VIEW | 2002年
关键词：
D O I：
10.1007/10856518_54
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
High angular resolution is one of the key factors needed to detect and investigate young stars, their circumstellar environment and the possible presence of exoplanets. In this respect, the VLTI represents one of the most powerful tools available in the short term. We describe the phased implementation of the VLTI, from the basic configuration which has recently achieved first fringes, to the full array with all subsystems and complete instrumentation that will be operational in the next years. We provide examples of techniques for the study of young stars and exoplanets.
引用
收藏
页码：416 / 421
页数：6
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