Relative spectrophotometry of Comet Halley in the near-IR region

Details Relative spectrophotometry of Comet Halley in the near-IR region Relative spectrophotometry of Comet Halley in the near-IR region

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991avest..25..599e&link_type=abstract

Astronomicheskii Vestnik (ISSN 0320-930X), vol. 25, Sept.-Oct. 1991, p. 599-602. In Russian.

Astronomy and Astrophysics

Astronomy

Astronomical Photometry, Astronomical Spectroscopy, Halley'S Comet, Near Infrared Radiation, Carbon Monoxide, Cyano Compounds, Infrared Astronomy, Spectral Energy Distribution, Spectrum Analysis

Scientific paper

Five photographs were chosen from a series of spectrograms of the NIR region of Comet Halley in the 6000-9000-A interval. The molecular bands CO (3-0), (4-1), (10-2), (11-3); H2O(+) (0,7,0),(0,6,0) NH2 (0,6,0) (0,5,0); and CN (2-0), (3-1), (4-2), (5-3) in the red system and C2 (2-0) in the Phillips system were identified. An asymmetrical distribution from cross sections of CN was detected; it is explained by the effect of jets in the circumnuclear region.

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