Optical spectroscopy of the coma of Comet Halley at ESO

Details Optical spectroscopy of the coma of Comet Halley at ESO Optical spectroscopy of the coma of Comet Halley at ESO

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986msngr..44...15f&link_type=abstract

ESO Messenger (ISSN 0722-6691), June 1986, v. 44, p. 15, 16.

Astronomy and Astrophysics

Astronomy

Astronomical Spectroscopy, Comet Nuclei, Halley'S Comet, Visible Spectrum, Radiation Distribution, Solar Radiation

Scientific paper

Using optical spectra (3550-6800 A) obtained with the 1.5-m University of Bologna telescope for the preperihelion phase, and with the 1.52-m ESO telescope for the postperihelion phase, the coma of Comet Halley is studied. A total of 25 spectra were obtained with different slit orientations and exposure times. The observed extension of the scattered solar radiation implies a very extended dust component.

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