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The population of bright NEAs

Published online by Cambridge University Press:  05 March 2015

G. B. Valsecchi  and
G. F. Gronchi
G. B. Valsecchi
Affiliation:
IAPS-INAF, Roma, Italy IFAC-CNR, Sesto Fiorentino, Italy
G. F. Gronchi
Affiliation:
University of Pisa, Pisa, Italy
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Our understanding of the orbital distribution of NEAs is influenced by discovery selection effects, so that it is likely that the orbital distribution of known NEAs differs from the true distribution. In fact, our ability to reconstruct the true distribution critically depends on the removal of discovery biases from the known population.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Highlights H16: Highlights of Astronomy , August 2012 , pp. 492 - 493
Copyright
Copyright © International Astronomical Union 2015 

References

Bottke, W. F., Morbidelli, A., Jedicke, R., Petit, J.-M., Levison, H. F., Michel, P., & Metcalfe, T. S. 2002, Icarus 156, 399CrossRefGoogle Scholar
Gronchi, G. F. & Milani, A. 2001, Icarus 152, 58Google Scholar
Jedicke, R. 1996, AJ 111, 970CrossRefGoogle Scholar