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A study of asteroid pole-latitude distribution based on an extended set of shape models derived by the lightcurve inversion method
- 1.0365932 - ASÚ 2012 RIV FR eng J - Journal Article
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
R&D Projects: GA ČR GD205/08/H005
Institutional research plan: CEZ:AV0Z10030501
Keywords : minor planets * photometric thechniques * numerical methods
Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics
Impact factor: 4.587, year: 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.
Permanent Link: http://hdl.handle.net/11104/0201059
Number of the records: 1