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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)
( 1) M.P.C.13641
( 2) Milani, A. et al. (1989) Icarus 78, 212-269. (Dynamics of planet-crossing asteroids - Classes of orbital behavior - project Spaceguard)
( 3) Hahn, G. & C.-I. Lagerkvist (1988) Celest. Mech. 43, 285-302. (Orbital evolution studies of planet-crossing asteroids)
( 4) Hahn, G. & C.-I. Lagerkvist (1988) in "The Few Body Problem" (Ed.M.J. Valtonen), Kluwer Acad. Publ., Dordrecht, Netherlands, pp. 143-146. (Long-term orbital evolution studies of Aten-Apollo-A mor objects)
( 5) Janiczek, P.M. et al. (1972) Astron. J. 77, 764-773. (Resonances and Encounters in the Inner Solar System)
( 6) Antal, M. (1974) I.A.U.C. 2648. (887 Alinda, photographic photometry)
( 7) Hodgson, R.G. (1974) MPB 1, 36-37. (Observations of 887 Alinda)
( 8) Lazzarin, M. et al. (2004) Icarus 169, 373-384. (Visible and near-infrared spectroscopic investigation of near-Earth objects at ESO: first results)
( 9) Binzel, R.P. et al. (2004) Icarus 170, 259-294. (Observed spectral properties of near-Earth objects: results for population distribution, source regions, and space weathering processes.)
(10) 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)
(11) 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)
(12) Krugly, Yu. N. et al. (2002) Proceedings of ACM2002, ESA-SP500, pp. 903-906. (CCD photometry of Near-Earth asteroids in 2001) (rot.per. for 719,1916,26760,33342 2001 MF1; LCs for 1620,3103,55 87,1999 KW4)
(13) Petr Pravec's Ondrejov NEO Photometric Program Webpage
(14) R. Behrend Courbes des lumiere, Observatoire de Geneve website
(15) Lazzarin, M. et al. (2004) Icarus 169, 373-384. (Visible and near-infrared spectroscopic investigation of near-Earth objects at ESO: first results)
(16) Binzel, R.P. et al. (2004) Icarus 170, 259-294. (Observed spectral properties of near-Earth objects: results for population distribution, source regions, and space weathering processes.)
NEODyS Page of ( 719) Albert