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* - orbital type derived from osculating orbital elements
# - absolute magnitude H derived from astrometric observation via orbit determination - G value assumed to be 0.15
! - quality code according to Lagerkvist et al. (1989) in "Asteroids II" (Eds. R.P.Binzel et al.), Univ.Ariz.Press, Tucson, USA, pp. 1162-1179.
(001) M.P.E.C. 2000-E23
(002) Hirabayashi, M. et al. (2010) Icarus 206, 780-782. (Linear stability of collinear equilibrium points around an asteroid as a two-connected-mass: Application to fast rotating Asteroid 2000EB14)
(003) Binzel, R.P. et al. (2002) in "Asteroids III" (Eds. W.F.Bottke et al.), Univ.Ariz.Press, Tucson, USA, pp. 255-271. (Physical Properties of NEOs)
(004) Binzel, R.P. et al. (2002) in "Asteroids III" (Eds. W.F.Bottke et al.), Univ.Ariz.Press, Tucson, USA, pp. 255-271. (Physical Properties of NEOs)
(005) Whiteley, R.J. et al. (2002) Proceedings of ACM2002, ESA-SP500, pp. 473-480. (Monolithic fast-rotating asteroids) (H-values and rotation properties of 36 NEAs)
(006) Whiteley, R.J. et al. (2000) B.A.A.S. 32, 1003. (Lightcurve analysis of 4 monolithic fast-rotating asteroids.) (2000 AG6, 2000 DO8, 2000 EB14, 2000 HB24)
(007) Whiteley, R.J. et al. (2002) Icarus 157, 139-154. (Lightcurve Analysis of Four New Monolithic Fast-Rotating Asteroids) (2000 AG6,2000 DO8, 2000 EB14,2000 HB24)
(008) Whiteley, R.J. et al. (2002) Proceedings of ACM2002, ESA-SP500, pp. 473-480. (Monolithic fast-rotating asteroids) (H-values and rotation properties of 36 NEAs)
NEODyS Page of 2000 EB14