Abstract
Modern astronomy includes optical, ultraviolet, infrared and, in recent years, radio, γ-ray, and X-ray astronomy. Such a classification is justified to a certain degree. In fact, the difference in wavelength ranges causes a distinction in the methods and techniques of receiving radiation. Also, the solution of specific problems requires observation in different wavelength regions. In this respect it is possible to describe a new astronomical branch, the submillimeter one.
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Salomonovič, A.E. (1968). Some Problems and Instrumental Features of Submillimeter Astronomy. In: Perek, L. (eds) Highlights of Astronomy. International Astronomical Union / Union Astronomique Internationale, vol 1. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-3417-3_11
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