On the observability of radiation forces acting on near-Earth asteroids

[1]  M. N. Meshkov,et al.  Radar observations and physical model of asteroid 6489 Golevka , 2000 .

[2]  Andrea Milani,et al.  Yarkovsky Effect on Small Near-Earth Asteroids: Mathematical Formulation and Examples , 2000 .

[3]  A. Milani,et al.  Direct solar radiation pressure on the orbits of small near-Earth asteroids: observable effects? , 2000 .

[4]  P. Farinella,et al.  The Yarkovsky Seasonal Effect on Asteroidal Fragments: A Nonlinearized Theory for Spherical Bodies , 1999 .

[5]  M. Kocifaj,et al.  Real Dust Particles and Unimportance of the Poynting-Robertson Effect , 1999, astro-ph/9910042.

[6]  D. Vokrouhlický A COMPLETE LINEAR MODEL FOR THE YARKOVSKY THERMAL FORCE ON SPHERICAL ASTEROID FRAGMENTS , 1999 .

[7]  D. Vokrouhlický,et al.  The Yarkovsky Seasonal Effect on Asteroidal Fragments: A Nonlinearized Theory for the Plane-parallel Case , 1998 .

[8]  D. Vokrouhlický Diurnal Yarkovsky effect as a source of mobility of meter-sized asteroidal fragments. I. Linear theory , 1998 .

[9]  G. Angelis Asteroid spin, pole and shape determinations , 1995 .

[10]  D. Rubincam,et al.  Asteroid orbit evolution due to thermal drag , 1995 .

[11]  D. Matson,et al.  Radiometry of near-earth asteroids. , 1989, The Astronomical journal.

[12]  J. Burns,et al.  Radiation forces on small particles in the solar system , 1979 .

[13]  D. Vokrouhlický DIURNAL YARKOVSKY EFFECT AS A SOURCE OF MOBILITY OF METER-SIZED ASTEROIDALFRAGMENTS : II. NON-SPHERICITY EFFECTS , 1998 .