Asteroid models from combined sparse and dense photometric data

التفاصيل البيبلوغرافية
العنوان: Asteroid models from combined sparse and dense photometric data
المؤلفون: Ďurech, J., Kaasalainen, M., Warner, B. D., Fauerbach, M., Marks, S. A., Fauvaud, S., Fauvaud, M., Vugnon, J.-M., Pilcher, F., Bernasconi, L., Behrend, R., Ďurech, J., Kaasalainen, M., Warner, B. D., Fauerbach, M., Marks, S. A., Fauvaud, S., Fauvaud, M., Vugnon, J.-M., Pilcher, F., Bernasconi, L., Behrend, R.
المصدر: Astronomy and Astrophysics; January 2009, Vol. 493 Issue: 1 p291-297, 7p
مستخلص: Aims. Shape and spin state are basic physical characteristics of an asteroid. They can be derived from disc-integrated photometry by the lightcurve inversion method. Increasing the number of asteroids with known basic physical properties is necessary to better understand the nature of individual objects as well as for studies of the whole asteroid population.
قاعدة البيانات: Supplemental Index
الوصف
تدمد:00046361
14320746
DOI:10.1051/0004-6361:200810393