Bibcode
Székely, P.; Kiss, L. L.; Szabó, Gy. M.; Sárneczky, K.; Csák, B.; Váradi, M.; Mészáros, Sz.
Bibliographical reference
Planetary and Space Science, Volume 53, Issue 9, p. 925-936.
Advertised on:
8
2005
Citations
6
Refereed citations
6
Description
We present CCD photometric observations of 23 main-belt asteroids, of
which 8 have never been observed before; thus, the data of these objects
are the first in the literature. The majority showed well-detectable
light variations, exceeding 0.1. We have
determined synodic periods for 756 Lilliana (9.36), 1270
Datura (3.4), 1400 Tirela (13.36), 1503 Kuopio
(9.98), 3682 Welther (3.59), 7505 Furushu
(4.14) and 11436 1969 QR (12.3), while uncertain
period estimates were possible for 469 Argentina (12.3), 546
Herodias (10.4) and 1026 Ingrid (5.3). The shape
of the lightcurves of 3682 Welther changed on a short time-scale and
showed dimmings that might be attributed to eclipses in a binary system.
For the remaining objects, only lower limits of the periods and
amplitudes were concluded.