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100-MICRON Survey of the Galactic Plane

W. F. Hoffmann, Carl L. Fredrick, Roger J. Emery

Open publisher page 57 citations

Abstract

A survey of a portion of the galactic plane has been carried out at a wavelength of 100 with a beamwidth of 12' and a sensitivity of 1022 W Hz-i. The survey covers 750 square degrees of the sky including most of the galactic plane between t11 = 335 and tIl - 88 and a number of other selected areas of interest. Seventy-two sources have been detected, 60 of which are identified with continuum radio sources, bright nebulae, dark nebulae, and infrared stars.

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What this paper is about

A survey of a portion of the galactic plane has been carried out at a wavelength of 100 with a beamwidth of 12' and a sensitivity of 1022 W Hz-i. The survey covers 750 square degrees of the sky including most of the galactic plane between t11 = 335 and tIl - 88 and a number of other selected areas of interest. Seventy-two sources have been detected, 60 of which are identified with continuum radio sources, bright nebulae, dark nebulae, and infrared stars.

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OpenAlex reports 57 citations for this work. Citation counts describe recorded attention and do not establish research quality.

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Available abstract

A survey of a portion of the galactic plane has been carried out at a wavelength of 100 with a beamwidth of 12' and a sensitivity of 1022 W Hz-i. The survey covers 750 square degrees of the sky including most of the galactic plane between t11 = 335 and tIl - 88 and a number of other selected areas of interest. Seventy-two sources have been detected, 60 of which are identified with continuum radio sources, bright nebulae, dark nebulae, and infrared stars.

Key concepts: Physics, Galactic plane, Astrophysics, Sky, Stars, Astronomy

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