Abstract
Differential CCD photometry of three asteroids - 624 Hektor, 1167 Dubiago and 2060 Chiron - were carried out using the 2.5-m Nordic Optical Telescope on La Palma between 1990 March 14-17. From the resulting light curves the rotation period of Dubiago was obtained for the first time and found to be 14h3 ±0h1, while the previously reported rotation periods for Hektor (6h921) and Chiron (5h92) are consistent with our results. Light curve amplitudes of 0.22 ±0.02 mag for Hektor, 0.23 ± 0.02 mag for Dubiago and 0.07 ± 0.02 mag for Chiron were derived.
| Original language | English |
|---|---|
| Pages (from-to) | 115-118 |
| Number of pages | 4 |
| Journal | Monthly Notices of the Royal Astronomical Society |
| Volume | 250 |
| Issue number | 1 |
| Publication status | Published - 01 Jan 1991 |
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science
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