The Statistical Asteroid Model. I. The Main-Belt Population for Diameters Greater than 1 Kilometer
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Alberto Cellino | Vincenzo Zappala | E. F. Tedesco | A. Cellino | E. Tedesco | V. Zappalà | V. Zappalá
[1] Edward F. Tedesco,et al. The Infrared Space Observatory Deep Asteroid Search , 2002 .
[2] Morbidelli,et al. Origin of multikilometer earth- and mars-crossing asteroids: A quantitative simulation , 1998, Science.
[3] Paolo Tanga,et al. On the Size Distribution of Asteroid Families: The Role of Geometry , 1999 .
[4] Alessandro Morbidelli,et al. The shallow magnitude distribution of asteroid families , 2003 .
[5] Z. Ivezic,et al. Solar system objects observed in the Sloan Digital Sky Survey commissioning data , 2001 .
[6] Alberto Cellino,et al. Asteroid Families: Search of a 12,487-Asteroid Sample Using Two Different Clustering Techniques , 1995 .
[7] R. Jedicke,et al. The Orbital and Absolute Magnitude Distributions of Main Belt Asteroids , 1998 .
[8] Brett James Gladman,et al. Asteroid Showers on Earth after Family Breakup Events , 1998 .
[9] Richard J. Greenberg,et al. Numerical Evaluation of the General Yarkovsky Effect: Effects on Eccentricity and Longitude of Periapse , 2002 .
[10] P. Tanga,et al. Collisions and Gravitational Reaccumulation: Forming Asteroid Families and Satellites , 2001, Science.
[11] S. Dermott,et al. The Collisional Evolution of the Asteroid Belt and Its Contribution to the Zodiacal Cloud , 1997 .
[12] Paolo Tanga,et al. The Velocity–Size Relationship for Members of Asteroid Families and Implications for the Physics of Catastrophic Collisions , 1999 .
[13] Alessandro Morbidelli,et al. The Flora Family: A Case of the Dynamically Dispersed Collisional Swarm? , 2002 .
[14] Alberto Cellino,et al. Interlopers within Asteroid Families , 1995 .
[15] Aldo dell'Oro,et al. Asteroid families: open problems , 2004 .
[16] Robert Jedicke,et al. From Magnitudes to Diameters: The Albedo Distribution of Near Earth Objects and the Earth Collision Hazard , 2002 .
[17] István Csabai,et al. Comparison of Positions and Magnitudes of Asteroids Observed in the Sloan Digital Sky Survey with Those Predicted for Known Asteroids , 2002 .
[18] A. Cellino,et al. The Role of Families in Determining Collision Probability in the Asteroid Main Belt , 2001 .
[19] S. D. Price,et al. Space-based infrared near-Earth asteroid survey simulation , 2000 .
[20] Robert Jedicke,et al. Collisional Models and Scaling Laws: A New Interpretation of the Shape of the Main-Belt Asteroid Size Distribution☆ , 1998 .
[21] Francesco Marzari,et al. Collisional Evolution of Asteroid Families , 1995 .
[22] E. Tedesco,et al. Compositional Structure of the Asteroid Belt , 1982, Science.
[23] Comparison of Asteroids Observed in the SDSS with a Catalog of Known Asteroids , 2002, astro-ph/0202468.
[24] P. Michel. Secular Resonances: Transport Mechanism to Earth—Crossing Orbits , 1999 .
[25] Alain Doressoundiram,et al. The puzzling case of the Nysa-Polana family finally solved ? , 1998 .
[26] Paolo Tanga,et al. Estimated Abundance of Atens and Asteroids Evolving on Orbits between Earth and Sun , 2000 .
[27] K. Muinonen. Discovery and follow-up simulations for small Earth-crossing asteroids , 1998 .
[28] D. Padgett,et al. Asteroid Trails in Hubble Space TelescopeWFPC2 Images: First Results☆☆☆ , 1998 .
[29] C. J. van Houten,et al. Survey of Asteroids. , 1958 .
[30] A. McEwen,et al. Galileo Encounter with 951 Gaspra: First Pictures of an Asteroid , 1992, Science.
[31] P. Farinella,et al. Wavy size distributions for collisional systems with a small-size cutoff , 1994 .
[32] R. G. Hutton,et al. Polarimetric Observations of Small Asteroids: Preliminary Results , 1999 .
[33] A. Roy,et al. The Dynamics of Small Bodies in the Solar System , 1999 .
[34] Stephan D. Price,et al. The Supplemental IRAS Minor Planet Survey , 2002 .
[35] Alberto Cellino,et al. The size distribution of main-belt asteroids from IRAS data , 1991 .
[36] C. Grillmair,et al. The Spitzer First Look Survey—Ecliptic Plane Component: Asteroids and Zodiacal Background , 2004 .
[37] A. Ignatiev. Space Resources Roundtable 2 , 2000 .
[38] J. Weiland,et al. The Three-Dimensional Structure of the Zodiacal Dust Bands , 1997 .