Physical observations of comets: Their composition, origin and evolution

Details Physical observations of comets: Their composition, origin and evolution Physical observations of comets: Their composition, origin and evolution

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991plas.rept..151c&link_type=abstract

In NASA, Washington, Reports of Planetary Astronomy, 1991 p 151-152 (SEE N92-12792 03-89)

Astronomy and Astrophysics

Astronomy

Astronomical Spectroscopy, Chemical Composition, Comets, Near Ultraviolet Radiation, Space Observations (From Earth), Cn Emission, Iue, Schwassmann-Wachmann Comet, Spectral Bands, Spectrographs

Scientific paper

Observations of Comet P/Schwassmann-Wachmann 1 (SW1) during one observing run each in 1989 and 1990 are discussed, and the new significant information that was obtained is presented. Also discussed are near-UV observations of comets. The near-UV is a mostly unexplored spectral region for comets since it is not visible to spacecraft such as IUE and most ground-based detectors and spectrographs are not sensitive in the near-UV.

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