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Radio flare on η Gemini Star

Published online by Cambridge University Press:  23 September 2016

P.M. Herouni  and
V.S. Oskanian
P.M. Herouni
Affiliation:
Radiophysical Measurment Institute Armenian Academy of Sciences, USSR
V.S. Oskanian
Affiliation:
Radiophysical Measurment Institute Armenian Academy of Sciences, USSR

Extract

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The first at the world Radio-Optical Telescope ROT-32/54/2, 6 was mounted on the southern slope of Mount Aragats in Armenia at 1700 m above sea level. The Large Antenna of ROT with the unmovable hemisperical main mirror of 54 m in diameter and movable small correcting mirror is the extremely accurate and shortwave (down to 1 mm). Using aperture is 32m. The diameter of the Optical Telescope is 2.6 m. General view of ROT is shown in Fig.1.

Type
I Flare Stars Optical Observations and Flare Statistics
Information
Symposium - International Astronomical Union , Volume 137: Flare Stars in Star Clusters, Association and Solar Vicinity , 1990 , pp. 145 - 146
Copyright
Copyright © Kluwer 1990 

References

Referenses

1. Herouni, P.M. (1986) ‘Radiooptical Telescope ROT-32/54/2,6’, XVIII All-Union Conference of Radioastronomy, Proc.1, Irkutsk, pp. 5–7.Google Scholar
2. Kholopov, P.N. et. al. (1985) ‘General Catalogue of Variable Stars’,Vol.2, Nauka, Moscow.Google Scholar