Photoelectric photometry of the minor planets 41 Daphne and 129 Antigone

Details Photoelectric photometry of the minor planets 41 Daphne and 129 Antigone Photoelectric photometry of the minor planets 41 Daphne and 129 Antigone

Apr 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977a%26a....56....7s&link_type=abstract

Astronomy and Astrophysics, vol. 56, no. 1-2, Apr. 1977, p. 7-11.

Astronomy and Astrophysics

Astrophysics

8

Asteroids, Astronomical Photometry, Light Curve, Atmospheric Attenuation, Least Squares Method, Tables (Data), Ubv Spectra

Scientific paper

Photometric observations of 41 Daphne and 129 Antigone were made during
the period April-June 1976. The synodic periods of rotation are 0.249492
and 0.206548 day, respectively. The absolute magnitudes and phase
coefficients are deduced by a linear magnitude-phase relation.

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