Submillimeter astronomy at the NASA/University of Hawaii 3-meter infrared telescope facility

Details Submillimeter astronomy at the NASA/University of Hawaii 3-meter infrared telescope facility Submillimeter astronomy at the NASA/University of Hawaii 3-meter infrared telescope facility

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983stin...8417083.&link_type=abstract

Final Report, 1 Oct. 1979 - 31 Oct. 1983 Chicago Univ., IL. Fermi Inst.

Astronomy and Astrophysics

Astronomy

Astronomical Photometry, Brightness Temperature, Infrared Astronomy, Photometers, Planetary Atmospheres, Submillimeter Waves, Cryogenic Cooling, Globules, Jupiter (Planet), Neptune (Planet), Reflection Nebulae, Saturn Rings, Titan, Uranus (Planet)

Scientific paper

Problems encountered in the design of a submillimeter photometer for the infrared telescope facility and some of the solutions already provided are described. Observations of Saturn's rings and the determination of the brightness temperature of Titan, Jupiter, Saturn, Neptune, and Uranus are summarized. Significant findings during solar, galactic, and extragalactic observations include the discovery of low luminosity star formation in the Bok Globule B335 and determination of the far infrared properties of dust in the reflection nebula NGC 7023.

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