Possibilities for Studying Star-Formation Processes at IRAO ‘‘Suffa’’: Objects and Tasks
A. S. HojaevUlugh Beg Astronomical Institute of the Uzbek Academy of Sciences, 100052, Tashkent, UzbekistanИ. И. ЗинченкоFederal research center A. V. Gaponov-Grekhov Institute of Applied Physics of the Russian Academy of Sciences, 603950, Nizhny Novgorod, Russia
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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.
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