Infrared photometry of Comet Kohoutek

Details Infrared photometry of Comet Kohoutek Infrared photometry of Comet Kohoutek

Dec 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974icar...23..577z&link_type=abstract

Icarus, vol. 23, Dec. 1974, p. 577-579.

Astronomy and Astrophysics

Astronomy

6

Astronomical Photometry, Bolometers, Infrared Astronomy, Infrared Photometry, Kohoutek Comet, Brightness Temperature, Calibrating, Coma, Comet Tails, Infrared Radiation, Interplanetary Dust, Luminous Intensity, Spectral Energy Distribution, Telescopes

Scientific paper

The Comet Kohoutek was observed from 8.8 to 21 microns using the 1.3-m telescope at Kitt Peak National Observatory in December, 1973, and January, 1974. Data are given on the infrared fluxes observed in the 24-arcsec beam, brightness temperatures, color temperatures, and the derived infrared luminosity. The results show that Kohoutek is a bright infrared source, and are consistent with infrared observations of other comets.

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