A study of asteroid pole-latitude distribution based on an extended set of shape models derived by the lightcurve inversion method

0365932 - ASÚ 2012 RIV FR eng J - Článek v odborném periodiku
Hanuš, J. - Ďurech, J. - Broz, M. - Warner, B. D. - Pilcher, F. - Stephens, R. - Oey, J. - Bernasconi, L. - Casulli, S. - Behrend, R. - Polishook, D. - Henych, Tomáš - Lehký, L. - Yoshida, F. - Ito, T.
A study of asteroid pole-latitude distribution based on an extended set of shape models derived by the lightcurve inversion method.
Astronomy & Astrophysics. Roč. 530, June (2011), A134/1-A134/16. ISSN 0004-6361. E-ISSN 1432-0746
Grant CEP: GA ČR GD205/08/H005
Výzkumný záměr: CEZ:AV0Z10030501
Klíčová slova: minor planets * photometric thechniques * numerical methods
Kód oboru RIV: BN - Astronomie a nebeská mechanika, astrofyzika
Impakt faktor: 4.587, rok: 2011

Tens of thousands of sparse-in-time lightcurves from astrometric projects are publicly available. We investigate these data and use them in the lightcurve inversion method to derive new asteroid models. By having a greater number of models with known physical properties, we can gain a better insight into the nature of individual objects and into the whole asteroid population.
Trvalý link: http://hdl.handle.net/11104/0201059