Submillimeter spectrophotometry in the Pamirs

Details Submillimeter spectrophotometry in the Pamirs Submillimeter spectrophotometry in the Pamirs

Jul 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pazh...15..667m&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 15, July 1989, p. 667-672. In Russian. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

Astronomical Spectroscopy, Brightness Distribution, Brightness Temperature, Infrared Astronomy, Spectrophotometry, Bolometers, Calibrating, Cosmic Dust, Galaxies, Interstellar Matter, Planets

Scientific paper

Observations of planets, interstellar molecular-dust clouds (zones of active star formation), and galaxies were carried out at several submillimeter-range wavelengths mainly in the 0.34 mm 'transparency window'. The brightness temperatures were measured and the parameters of the brightness distribution of the radiation in the extended sources were estimated. For the brightest sources, the results are in agreement with measurements obtained earlier.

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