Investigation of gas and dust production in Comet Halley on the basis of ground-based spectrophotometry

Details Investigation of gas and dust production in Comet Halley on the basis of ground-based spectrophotometry Investigation of gas and dust production in Comet Halley on the basis of ground-based spectrophotometry

Aug 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989kfnt....5...38s&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 5, July-Aug. 1989, p. 38-44. In Russian.

Other

Astronomical Photometry, Halley'S Comet, Interplanetary Dust, Outgassing, Spectrophotometry, Bandwidth, Carbon, Cn Emission, Molecular Gases, Particle Production

Scientific paper

The production rate (Q) of CN, C2, C3, and dust in Comet Halley was calculated based on spectrophotometric observations performed at the Shemakha Observatory during December 1985 and January 1986. The Q(CN)-Q(C2) and Q(CN)-Q(C3) diagrams are constructed for Comet Halley and 17 periodic and nonperiodic comets. It is shown that the core of Comet Halley is compositionally homogeneous and, from this point of view, does not differ essentially from that of the other comets investigated.

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