Possibilities for Studying Star-Formation Processes at IRAO ‘‘Suffa’’: Objects and Tasks

IF 1.3 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS
A. S. Hojaev, I. I. Zinchenko
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引用次数: 0

Abstract

We describe the general remaining unclear issues of the star-formation process that could be studied using the millimeter radio telescope on the Suffa plateau (Uzbekistan). A description of possible objects of study is given. The possibilities of solving scientific problems in studying these objects using various instruments are assessed: the 70-m RT-70 radio telescope, a smaller-diameter antenna (15–20 m), and an antenna array consisting of small (3–8 m) antennas.

在IRAO“Suffa”研究恒星形成过程的可能性:对象和任务
我们描述了在苏法高原(乌兹别克斯坦)使用毫米射电望远镜可以研究的恒星形成过程中一般仍然不清楚的问题。对可能的研究对象进行了描述。评估了使用各种仪器解决研究这些天体的科学问题的可能性:70米RT-70射电望远镜,较小直径的天线(15-20米)和由较小(3-8米)天线组成的天线阵列。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Astrophysical Bulletin
Astrophysical Bulletin 地学天文-天文与天体物理
CiteScore
2.00
自引率
33.30%
发文量
31
审稿时长
>12 weeks
期刊介绍: Astrophysical Bulletin is an international peer reviewed journal that publishes the results of original research in various areas of modern astronomy and astrophysics, including observational and theoretical astrophysics, physics of the Sun, radio astronomy, stellar astronomy, extragalactic astronomy, cosmology, and astronomy methods and instrumentation.
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