Virtual Observatory for stellar astronomy

被引：1
|
作者：
Malkov, O. [1 ,2 ,3 ]
Zolotukhin, I. [4 ,5 ]
机构：
[1] Russian Acad Sci, Inst Astron, Moscow 119017, Russia
[2] Moscow MV Lomonosov State Univ, Fac Phys, Moscow 119992, Russia
[3] Univ Santiago de Compostela, Observ Astron Ramon Maria Aller, E-15782 Santiago De Compostela, Spain
[4] Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Moscow 119992, Russia
[5] CNRS, Observ Paris, LERMA, F-75014 Paris, France
来源：
ASTRONOMISCHE NACHRICHTEN | 2013年 / 334卷 / 08期
基金：
俄罗斯基础研究基金会;
关键词：
astronomical databases: miscellaneous; stars: fundamental parameters; LARGE MULTIBAND SURVEYS; BINARY STAR DATABASE; AUTOMATED SEARCH; OPEN CLUSTERS; DISCOVERY; TOOLS; BDB;
D O I：
10.1002/asna.201311929
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The principal idea of the Virtual Observatory is to achieve real transparency for astronomical data, similar to transparency for all the world's documents in the World Wide Web. In the Virtual Observatory, all the world's astronomical data is available from one's desktop. All archives understand the same query language, can be accessed through a uniform interface, and diverse data can be analyzed with the same tools. In particular, facilities of the Virtual Observatory allow users to make a fast and correct analysis of objects from various surveys. It yields multi-photometry data on registered objects and makes it possible to determine stellar parameters. Methods of astronomical data analysis as well as their application to various areas of stellar astronomy are discussed in this paper. (c) 2013 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim
引用
收藏
页码：818 / 822
页数：5
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