Variability of P/Halley

Details Variability of P/Halley Variability of P/Halley

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...138l...9w&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 138, no. 1, Sept. 1984, p. L9, L10.

Physics

Optics

24

Astrometry, Astronomical Photometry, Halley'S Comet, Cassegrain Optics, Charge Coupled Devices, Image Processing, Telescopes, Variability, Comets, Halley, Photometry, Magnitude, Astronomy, Observations, Periods, Rotation, Astrometry, Short Period Comets, Procedure, Data

Scientific paper

Twenty-one photometric magnitudes of P/Halley (1982 i) have been measured on Jan. 27-30, 1984 with the Danish 1.5 m telescope at La Silla and a CCD. They have r.m.s. of + or 0.2 mag, and show night-to-night variability. The available material does not allow an unambiguous determination of a period of rotation, but short periods (not greater than 10 hours) are considered less likely.

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