The ultraviolet spectrum of Comet Seargent 1978m

Details The ultraviolet spectrum of Comet Seargent 1978m The ultraviolet spectrum of Comet Seargent 1978m

Mar 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979a%26a....73l...7j&link_type=abstract

Astronomy and Astrophysics, vol. 73, no. 1-2, Mar. 1979, p. L7-L9.

Astronomy and Astrophysics

Astronomy

14

Astronomical Spectroscopy, Comets, Emission Spectra, Satellite Observation, Ultraviolet Spectra, H Lines, Hydroxyl Radicals, Iue, Spaceborne Astronomy, Carbon Monosulfide, Carbon Monoxide, Emissions, Ultraviolet, Spectrum, Seargent, Comet, Observations, Comets, Wavelengths, Carbon Dioxide, Absorption Spectra, Lyman-Alpha Radiation

Scientific paper

UV spectrograms of Comet Seargent (1978m) have been obtained with the IUE satellite in the low- (1.8-nm) and high- (0.1-nm) dispersion modes. In the long-wavelength region (189-340 nm) emission bands of OH, CS, CO2(+), NH, and CO(+) can be identified, and the rotational structure of OH could clearly be resolved. In the short-wavelength region (119-192 nm) emission lines of H(Lyman-alpha), O I, C I, and S I appear. These observations demonstrate that the IUE observatory can effectively be used to obtain high-quality spectra of comets as faint as ninth magnitude.

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