The variation in the brightness of Halley's comet from ground-based narrow-band photometry

Details The variation in the brightness of Halley's comet from ground-based narrow-band photometry The variation in the brightness of Halley's comet from ground-based narrow-band photometry

May 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987mnras.226p...1w&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 266, P1

Astronomy and Astrophysics

Astronomy

12

Brightness Distribution, Halley'S Comet, Light Curve, Astronomical Photometry, Ground Truth

Scientific paper

Observations of Halley's comet in the period 1986 March 13 - 18 and May
7 - 14 using narrow-band photometry are described. Using identical
methods to those of Millis & Schleicher (1986), the authors find
excellent agreement with their results confirming the existence of a
7.37 day periodicity in the emission rate.

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