High-resolution ground-based spectroscopy: where and how?

被引：0
|
作者：
Pallavicini, R [1 ]
机构：
[1] Osserv Astron Palermo, INAF, I-90134 Palermo, Italy
来源：
ASTRONOMISCHE NACHRICHTEN | 2002年 / 323卷 / 3-4期
关键词：
instrumentation; spectrographs;
D O I：
10.1002/1521-3994(200208)323:3/4<288::AID-ASNA288>3.0.CO;2-6
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
An overview is presented of high-resolution optical spectrographs in operation or under development at large telescopes, with emphasis on those facilities best suited for the study of late-type stars and stellar surface inhomogeneities, Plans for the development of new high-resolution spectroscopic instruments are discussed with emphasis on the ICE spectrograph for the PEPSI spectropolarimeter at the LBT.
引用
收藏
页码：288 / 293
页数：6
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