Difficult cases in photometric studies of asteroids

被引:0
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作者
Marciniak, Anna [1 ]
Pilcher, Frederick [2 ]
Oszkiewicz, Dagmara [1 ]
Bartczak, Przemyslaw [1 ]
Santana-Ross, Toni [1 ]
Kaminski, Krzysztof [1 ]
Urakawa, Seitaro [3 ]
Ogloza, Waldemar [4 ]
Fauvaud, Stephane [5 ,6 ]
Kankiewicz, Pawel [7 ]
Kudak, Viktor [8 ]
Zejmo, Michal [9 ]
Nishiyama, Kota [3 ]
Okumura, Shin-ichiro [3 ]
Nimura, Tokuhiro [3 ]
Hirsch, Roman [1 ]
Konstanciak, Izabella [1 ]
Tychoniec, Lukasz [1 ]
Figas, Michal [1 ]
机构
[1] Adam Mickiewicz Univ, Fac Phys, Astron Observ Inst, PL-60286 Poznan, Poland
[2] 4438 Organ Mesa Loop, Las Cruces, NM 88011 USA
[3] Japan Spaceguard Assoc, Bisei Spaceguard Ctr, 1716-3 Okura, Ibara, Okayama 7141411, Japan
[4] Pedagogical Univ, Mt Suhora Observ, Podchorazych 2, PL-30084 Krakow, Poland
[5] Observ Bois Bardon, F-16110 Taponnat, France
[6] Assoc T60, 14 Ave Edouard Belin, F-31400 Toulouse, France
[7] Jan Kochanowski Univ, Inst Phys, Astrophys Div, Swietokrzyska 15, PL-25406 Kielce, Poland
[8] Uzhgorod Natl Univ, Uzhgorod, Ukraine
[9] Univ Zielona Gora, Kepler Inst Astron, Lubuska 2, PL-65265 Zielona Gora, Poland
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中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a photometric campaign targeted at asteroids that display both long periods of rotation and small amplitudes of brightness variations. Our aim is to de bias available sample of spin and shape modelled asteroids and to correct previous wrong period determinations. Our newest findings are corrected period determinations for asteroids (279) Thule (P=23.896 +/- 0.005 h), (673) Edda (P=22.340 +/- 0.004 h), and (737) Arequipa (P=7.0259 +/- 0.0003 h). Supporting lightcurves are presented in this paper.
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页码:84 / 90
页数:7
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